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MUGHALS Since 1917

﷽

Strategic Assets Advisors (ISO 55000)

DEEP SPACE

MUGHALS's KAINAT Program

"Sharing The Divine Knowledge By Pondering The Universe"

﷽

"…وَمَا خَلَقۡنَا السَّمَآءَ وَالۡاَرۡضَ وَمَا بَيۡنَهُمَا بَاطِلًا…"

"...AND WE (THE ALLAH, THE MASTER CREATOR AND THE SUSTAINER) DID NOT CREATE THE HEAVEN AND THE EARTH AND THAT (ALL) BETWEEN THEM, AIMLESSLY....."  Divine Holy Book Al-Quran:  Chapter: 38-Verse: 27

All hyperlinks open new window

Group URLs:  ABOUT >> COSMOLOGY >> LEGAL ENTITIES

Last update: August 06, 2025, By Program Lead

Advancing Vision of

The Founder of The Islamic Republic of Pakistan

Mohammad Ali Jinnah

Deep-Space Transformational Research

Research Resources from Astrophysics to Spacetime Geometry

Based on the Divine Principles of

Astronomy; Biology; Chemistry; Embryology; Geology;

History; Mathematics; Meteorology; Philosophy; 

Physics; Physiology; and Zoology.

KAINAT Program Research Focus

Algorithm Optimization: AI Protocols

Moon to Deep Space Supply Chain

Cosmic Radiation

Deep Spacetime Geometry

Deep-Space Radiation Impact on Earth Climate

Lead Policy Advisor: Pacific Enterprises International Syndicate (PEIS) USA

R&D Project Lead: Afro Eurasian Coalition (AEC) LLC USA

AEC-PEIS NAICS Code: 541690; USA DOD CAGE CODE: Active

AEC-PEIS SIC Code: 87420501; PEIS  SA FCC FRN #: 0034792853

Program Lead: Mohammad Afzal Mirza, President, AEC LLC USA

Our Priority Focus Programs

Spacecrafts & Astronauts Materials

Workforce Skills Development

(Integrated fields of Quantum Physics, Mathematics, Biology, Chemistry, Mechanical & Electrical Engineering)

MUGHALS Strategic Project 

Earth Observation System Research (EOSR)

Prime Research Source: The Divine Holy Al-Quran

Divine Holy Al-Quran, 1400 Hundred Years Revealed: Surah 67 - Verse 3  

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"...ٱلَّذِى خَلَقَ سَبْعَ سَمَـٰوَٰتٍۢ طِبَاقًۭا ۖ مَّا تَرَىٰ فِى خَلْقِ ٱلرَّحْمَـٰنِ مِن تَفَـٰوُتٍۢ ۖ فَٱرْجِعِ ٱلْبَصَرَ هَلْ تَرَىٰ مِن فُطُورٍۢ ٣..."

"....He (The ALLAH, The ALL MIGHTY; The Creator; The Sustainer of The COSMIC) is the One Who Created Seven Heavens, One Above the Other. You Will Never See (Find) any Imperfection in the Creation of the Most Compassionate.1 So Look Again: do you see any flaws?...." 

Spiral Galaxies

Mind Blowing images of 19 Face-on Spiral Galaxies from the James Webb Space Telescope in Near- and Mid-infrared Light 

Source: NASA

Deep Space Radiation Environment

Outside of Low Earth Orbit (LEO), Earth’s Protective Magnetosphere no longer operates, resulting in a much higher flux of radiation. 

  • The Deep Space Radiation Environment Consists of Two Major Contributors: 

  • Galactic Cosmic Rays (GCRs), Low-flux but Highly Energetic.

  • Solar Radiation Storms (SRS), known as (SEP) Solar Particle Events. 

    • These Sun Bursts range in intensity, from benign to extremely dangerous. 

MUGHALS Research Priorities

Deep-Space Optical Navigation (DSON)

Cosmic Radiation

Space Navigational Systems

Spacecraft Optical Navigation 

Global Ecosystem Dynamics Investigation (GEDI) Program

MUGHALS' Ongoing Research

Cosmic Radiation 

Inter-Satellite Optical Systems

AI Adoption Strategy

Climate Modeling and Prediction

Infrared Remote Sensing 

Environmental Monitoring (air, land, water)

Disaster Risk Reduction and Management

Sustainable Development Goals (SDGs) Tracking

Solar Flare Impact on Earth

Space Radiation refers to the High-Energy Particles (primarily Protons, Helium Nuclei, and Heavier Atomic Nuclei (HZE ions) and Electromagnetic Radiation found throughout space, posing significant risks to spacecraft and astronauts. 

  • It primarily consists of Galactic Cosmic Rays, Solar Energetic Particles, and particles trapped within Planetary Magnetic Fields. 

    • Understanding and Mitigating these Radiation Hazards is crucial for safe Space Exploration.  

Image Credit: NASA

Prime Research Source: The Divine Holy Al-Quran

Additional Research Sources: Space Agencies of;

China: CNSA | EU: ESA | Pakistan: SUPARCO | Russia: RSA 

USA: NASA | USDA | US DOE | USGS | US NIH | NOAA

Contact: peis@themughals.net

    • On 7 July 2025, ESA established first Optical Communication Link with a Spacecraft in Deep Space. 

    • The link was made with NASA’s Deep Space Optical Communications (DSOC) experiment aboard its Psyche Mission, currently at a distance of 1.8 Astronomical Units, around 265 million km. 

Deep Space Exploration

"Must-Have Technologies"

  1. Earth based Support System 

  2. Material Science Labs focusing Self Healing Materials

  3. Solar Propulsion

  4. Deep Space Atomic Clock

  5. Spacecraft Propulsion System and Large Solar Sail

  6. Inter Spacecrafts Optical (Laser) Communications System 

  7. Integrated Optical Communication and Navigation System

  8. Space Missions Risk Mitigation System

Some Underlying Technologies

Infrared Remote Sensing

Geomagnetic Disturbance

Climate Risk Analytics

Electromagnetic Spectrum

Radiometric Resolution

Desert Hydrology Water

Light Detection and Ranging

Data Visualization Tools

Flood Risk Management

Earth Observation Technology

Earth Observation Technology (EOT) enables an improved understanding of the Earth as an integrated system. EOT includes the Multiple-Integrated-Technologies for gathering information about the Earth's Surface, Waters and Atmosphere via Ground-based, Airborne UAVs, and/or Satellite and Remote Sensing Platforms.

Space Domain Awareness (SDA) 

Enhancing Space Domain Awareness (SDA)

Technological Advancements - Challenges - Solutions

Next-generation Sensors:

  • Space-based vs. Ground-based: While ground-based sensors like telescopes and radars are critical for SDA, they have limitations such as Atmospheric Interference, daylight restrictions, and difficulty observing objects at higher altitudes. Space-based sensors, on the other hand, overcome many of these Limitations and provide better coverage, particularly for Geosynchronous Earth Orbit (GEO) objects.

Advanced Radar:

  • Deep-Space Advanced Radar Capability (DARC): The U.S. Space Force's DARC system, built by Northrop Grumman, aims to significantly improve radar surveillance at higher altitudes, including GEO and geostationary orbits. DARC is expected to come online in 2025 and will be able to monitor orbits above 35,000 km. 

    • The development of such systems, potentially with international partners, can enhance tracking capabilities and resilience.

Radio Frequency (RF) Sensing:

  • Persistent Custody: RF sensing can provide continuous tracking of satellites based on their unique RF signatures, even in orbits like GEO and during all weather conditions. 

    • This capability also helps in identifying potential interference, malfunctions, or abnormal behavior. 

    • Ground and space-based RF networks complement each other to create a comprehensive picture of spectrum usage.

Active Illumination:

  • Moving beyond passive observation, active illumination, such as using lasers, can improve characterization and tracking of space objects. The European Space Agency (ESA) is testing a ESA Laser Ranging Station that uses conventional lasers to illuminate satellites equipped with Retroreflectors for Daylight Observations.

Distributed Satellite Systems:

  • Enhanced RSO Identification and Orbit Determination: Distributed satellite systems equipped with intersatellite links can improve SDA capabilities by providing more precise, real-time orbit determination of Resident Space Objects (RSOs). 

    • Algorithms can integrate data exchanged between satellites within a formation, utilizing onboard receivers and star trackers to enhance the accuracy of RSO identification and orbit determination. 

Artificial intelligence and Machine Learning (AI/ML)

Data Fusion and Analysis:

  • AI algorithms can process vast amounts of data from diverse sources – including radar, optical, RF, and allied/commercial data – to generate comprehensive situational awareness, detect anomalies, and assess risks. This includes identifying potential collision risks and operational anomalies in real time.

Anomaly Detection and Classification:

  • AI/ML models can analyze satellite imagery and other data to identify unusual changes that deviate from normal patterns, helping to detect potential threats or malfunctions.

Automated Collision Avoidance and Trajectory Predictions:

  • AI-powered systems can analyze orbital trajectories and predict potential collisions, then generate and execute optimal maneuver plans to avoid them, reducing the workload for human operators and enhancing efficiency. 

    • AI models can also more accurately predict the orbital variability of debris by continuously adapting to various influencing factors.

Space Debris Mitigation:

  • AI can contribute to sustainable debris management by learning from new data, adapting strategies, and developing scalable solutions for debris removal and prevention. 

    • This includes assisting in the design of spacecraft with built-in deorbiting mechanisms and optimizing collision avoidance strategies. 

Data Sharing and International Collaboration

Standardized Data Formats:

    • Standardizing data formats for Space Situational Awareness (SSA) information is essential for data exchange and to avoid misunderstandings. This can be achieved through internationally recognized interface control documents, such as the Consultative Committee for Space Data Systems (CCSDS) Blue Books.

Data Sharing Principles:

    • The World Economic Forum suggests that SSA data and information should be open by default, in accordance with national laws and regulations. If access is restricted, a clear justification should be provided, and efforts should be made to modify the data to enable its release, supporting space safety and sustainability.

Collaborative Efforts:

    • International collaborations like the Resolute Sentinel exercises bring together space experts from various countries to train and collaborate on space operations. 

      • This aids in enhancing interoperability and strengthening partnerships among emerging space powers by utilizing commercial capabilities and encouraging open communication.

Unified Data Libraries:

    • Initiatives such as the U.S. Space Force's Unified Data Library aim to make Radar Sensor Data more accessible to users at different classification levels, enhancing data sharing and collaboration. 

Space Weather and Debris Mitigation

Space Weather Forecasting:

    • Machine learning techniques and neural networks can be used to identify and characterize space weather phenomena, improving the prediction of events like solar flares and coronal mass ejections.

Debris Removal Technologies:

    • Research and development efforts focus on active debris removal technologies, such as robotic systems for servicing or deorbiting defunct satellites. 

      1. This includes missions like NASA's OSAM-1, which aims to use AI-enabled robotic systems to service and refuel satellites, extending their lifespan and reducing the need for new launches, thereby minimizing debris generation. 

Other Important Considerations

Legal and Ethical Implications of AI:

    • The integration of AI into SDA raises concerns about potential malfunctions, jurisdiction over non-consensual debris removal, liability for AI technology-caused damages, and the weaponization of outer space's impact. 

      • One research paper suggests guiding principles for the responsible deployment of AI in space to address these issues.

Human-Machine Teaming:

    • While AI has significant potential for SDA, human expertise and judgment remain critical, especially when dealing with anomalies and uncertainties in the complex space environment. 

      • Combining AI with human expertise is key to managing the increasing complexity of space operations. 

MUGHALS' Experts are exploring these areas, for a more detailed understanding of the challenges and opportunities in enhancing SDA can be achieved. 

Technology, Lawful Collaboration, and Responsible Practices play a critical role in ensuring the long-term safety and sustainability of space.

Solar Storms Disrupt Earth Technologies

Laser Ranging Station

 A Laser Ranging Station is a facility equipped with powerful lasers and sophisticated detection systems used to precisely measure distances to targets, primarily satellites and the moon. 

  • These stations are crucial for various scientific and practical applications, including geodesy, geophysics, and fundamental research.

Real-World Case Studies

1. Izaña-1 (IZN-1) Station Acceptance and Commissioning

  • Case Study: The successful completion of the IZN-1 laser ranging station's testing and commissioning phase in February 2022 marked a significant step in ESA's space debris mitigation and technology development efforts.

  • Performance Metrics: The station's performance was validated by the ESA Optical and Laser Expert Centre and the ESA/ESOC Navigation Support Office, meeting the requirements to join the International Laser Ranging Service (ILRS) as an engineering station.

Source: ESA, NASA (.gov). 

2. Tracking Cooperative Targets

  • Case Study: IZN-1 routinely tracks satellites equipped with retroreflectors using a 150 mW laser, contributing to precise orbit determination and space debris monitoring.

  • Performance Metrics: The station's current performance allows for tracking of these cooperative targets with high accuracy, comparable to other high-performance ILRS stations.

Source: NASA (.gov). 

3. Passive optical observations of space debris

  • Case Study: IZN-1 also conducts passive optical observations of space debris, providing valuable data for space debris environment models.

  • Performance Metrics: These observations have led to the discovery of faint, lightweight objects with high area-to-mass ratios, which are likely pieces of thermal blankets from satellites.

Source: European Space Agency, NASA (.gov). 

4. Optical communications demonstrations

  • Case Study: IZN-1 serves as a testbed for advanced optical communication technologies, including demonstrating coarse and fine pointing capabilities and successfully coupling optical downlink signals into the station's receive optical path.

  • Performance Metrics: The station has successfully demonstrated coupling optical downlink signals in the C-band into the station's multimode fiber, a key step towards implementing future high-data-rate optical communications from low-Earth orbit satellites.

Source: NASA (.gov). 

5. Development of ground-based laser momentum transfer (LMT) concept

    • Case Study: A conceptual study on ground-based LMT to LEO space debris, funded by ESA and led by the German Aerospace Centre (DLR), explored the feasibility of using lasers to gently nudge debris objects out of busy orbital paths.

    • Performance Metrics: The study evaluated the achievable thrust on LEO debris objects with commercially available components and assessed the efficiency of the imposed thrust on collision probability.

Source: ScienceDirect.com. 

6. Space debris attitude determination

  • Case Study: ESA's Space Debris Office, in collaboration with research institutes like AIUB, FHR, HTG, and IWF, is investigating the use of SLR, passive optical, and radar imaging data to determine the attitude state and motion of debris (uncooperative objects) in LEO and GTO.

  • Performance Metrics: The project aims to provide representative data sets for selecting debris removal technologies and for developing mechanisms for determining attitude state in spacecraft contingencies.

Source: NASA (.gov). 

7. Deep-space optical communication NASA's Psyche mission

  • Case Study: ESA marked a historic milestone by establishing its first deep-space optical communication link with NASA's Deep Space Optical Communications (DSOC) experiment aboard its Psyche mission, currently at a distance of 1.8 astronomical units.

  • Performance Metrics: This demonstration highlights the potential for interoperability between ESA and NASA in optical communications and paves the way for higher data rates in deep space missions.

Source: European Space Agency. 

ESA's Space Safety Program  (S2P) Benefit Case Studies

    • Case Study: The S2P Program, which includes Laser Ranging Activities, aims to protect our planet and assets in space from hazards originating in space.

    • Performance Metrics: PwC's analysis of selected S2P activities demonstrates benefits in terms of innovation, industry competitiveness, and market opportunities, particularly in areas like space weather monitoring and collision avoidance.

Source: ESA Space Economy. 

Automation Collision Avoidance with Machine Learning

  • Case Study: ESA is developing a collision avoidance system that will leverage machine learning to automatically assess the risk of in-space collisions, improve decision-making processes, and potentially even send commands to at-risk satellites.

    • Performance Metrics: The system's ability to reduce false alarms, enhance the efficiency of collision avoidance maneuvers, and ultimately minimize debris creation will be crucial for protecting operational satellites.

Source: European Space Agency.

Mission: Tracking Space Weather Impact on Earth

"Conditions on the Sun and in the Solar Wind, Magnetosphere, Ionosphere and Thermosphere (Earth’s Atmosphere) can influence the performance and reliability of Space-Borne and Ground-Based Technological Systems (Electromagnetic Energy, Climate Change etc.) and can endanger Human Life, Health and Civilization."

Our Research Focus

Cosmic Radiation | Electromagnetic Pulse | Geomagnetic Disturbance | 

Spacetime Geometry | Space Weather | Solar Electric Propulsion

With satellites, airborne missions, shipboard measurements, and supercomputers, NASA and other institutions have been investigating the space for decades. 

Image Source: NASA

Image Source: NOAA

CONTACT

More from NASA

The Causes of Climate Change

What Is the Sun's Role in Climate Change?

There Is No Impending 'Mini Ice Age'

Climate Change: Incoming Sunlight (NOAA)

Earth's Energy Budget Remained Out of Balance Despite Unusually Low Solar Activity

The NASA EOS Project Science Office (EOSPSO) is bringing program information and resources to the Earth science research community and the general public alike. 

NASA’s Earth Observing System (EOS) is a coordinated series of polar-orbiting and low inclination satellites for long-term global observations of the land surface, biosphere, solid Earth, atmosphere, and oceans.

👉 The FCC/Public Safety and Homeland Security Bureau released a Public Notice seeking comment on any impact to communications believed to be a result of the May 2024 severe geomagnetic storm.  Comments are due 24 June 2024.  See link below and attached for the notice.  

Image Source: NASA

Image Source: UT Austin, USA

Image Source: NOAA

Image Source:  SWPC-NOAA

What Is the Solar Cycle?

Our Sun is a huge ball of electrically-charged hot gas. This charged gas moves, generating a powerful magnetic field. The Sun's magnetic field goes through a cycle, called the Solar Cycle.

Every 11 years or so, the Sun's Magnetic Field completely flips. This means that the Sun's north and south poles switch places. Then it takes about another 11 years for the Sun’s north and south poles to flip back again.

The Solar Cycle affects Activity on the surface of the Sun, such as Sunspots which are caused by the Sun's Magnetic Fields. As the magnetic fields change, so does the amount of activity on the Sun's surface.

One way to track the solar cycle is by counting the number of sunspots. The beginning of a solar cycle is a Solar Minimum, or when the Sun has the least sunspots. Over time, solar activity—and the number of sunspots - increases.

The middle of the solar cycle is the Solar Maximum, or when the Sun has the most sunspots. As the cycle ends, it fades back to the solar minimum and then a new cycle begins. Read more...

Solar Cycle Progression and Forecast

Electromagnetic Spectrum

Electromagnetic energy travels in waves and spans a broad spectrum from very long radio waves to very short gamma rays. You depend on electromagnetic energy every hour of every day. Without it, the world you know could not exist. 

Electromagnetic Pulse (EMP):  An Electromagnetic Pulse is a burst of Electromagnetic Energy produced by a nuclear explosion in the atmosphere, considered capable of widespread damage to power lines, telecommunications, and electronic equipment etc.

Geomagnetic Disturbance: A Geomagnetic Disturbance is a temporary disturbance of the Earth's magnetosphere caused by a solar wind shock wave and/or cloud of magnetic field that interacts with the Earth's Magnetic Field.

Dr. I. H. Usmani Ph.D.

ALLAH MAY KEEP ON BLESSING HIS SOUL. Ameen

Father of Pakistan Atomic and Space Program

Former Chairman (1962 to 1963), Board of Governors of the International Atomic Energy Agency (IAEA)

👉 1936, MSc Physics, Aligarh Muslim University, United India

👉 1939, PhD, age 26, Nuclear Physics (Electron Diffraction through Crystallization, a technique that uses an Electron Beam to determine the structure of a Material's Crystal Lattice), Imperial College London, UK

👉 1960, Engineered Peaceful and Commercial usage of the Nuclear Energy (Agriculture, Bioeconomy, Health, Material Sciences etc.)

👉 1963, on behalf of Pakistan worked on International Arms Control Partial Nuclear Test Ban Treaty (PTBT), signed by the United States, Great Britain, and the Soviet Union)

👉 1960 - 1970s, Environmental Impact, Climate Change, Solar Radiation Modification etc.

👉 1960 - 1971, Chairman Pakistan Atomic Energy Commission (@The_PAEC)

👉  1963, Chairman Board of Governors, International Atomic Energy Agency (@iaeaorg)

 👉  1986, War and Peace in the Nuclear Age; TV Interview

Dr. Bashir A. Syed, Sc.D.

ALLAH MAY KEEP ON BLESSING HIS SOUL. Ameen

Dr. Bashir A. Syed, Sc.D., (Died June 1st, 2015 in Houston, Texas USA) was Muslim-Pakistani-American Solar Physicist and a NASA Research Scientist in the field of Robotics and Solar Sciences. He was the member of New York Academy of Sciences.[1] 

He produced numerous innovative research articles on resolving the energy crises in the world[1]. Dr. Syed is attributed with establishing the Wind Energy and Solar Energy Plants in the Pakistan. He also inducted a separate research institutions on Solar Physics and Technology at Space & Upper Atmosphere Research Commission (@SuparcoOfficial) and Pakistan Atomic Energy Commission (@The_PAEC). 

Bashir Syed joined NASA in 1989 while working at General Electric USA. He was transferred to the International Space Station as a Solar Technologist.[2] As a NASA Scientist he worked in the United States Space Program. 

Dr. Syed played a major role in the project from the Design Phase till the Construction Phase. He also participated in the Space Shuttle Modification Program. 

Dr. Syed worked on the development of NASA's space probes. He is a specialist on Cosmic and Solar Radiation. As a result, Dr. Syed was In Charge of Space Radiation Effects on Space Craft and Their Components. Dr. Syed was heavily involved in the production and development of Mars Pathfinder. 

Dr. Syed also worked as an Astronaut Trainer and in the Astronaut Development Program. He also worked in the United States Mercury Project where he did research in Solar Produced Plasmas. Dr. Syed retired from NASA on September 22, 2002. He continued his research in the field of Microtechnology, especially Carbon Nanotubes.[2]

Portable Seismograph Technology

Portable Seismograph Technology centers around the use of small, lightweight Seismographs designed for rapid deployment and easy transport to various locations. These instruments are built to withstand field conditions and are valuable for recording Seismic Activity in diverse settings 

Core Principle: Portable Seismographs, like their larger counterparts, operate on the principle of Inertia. 

In seismology, Inertia is a fundamental concept that explains how instruments like seismometers detect and measure earthquakes. 

Earth Science Data Resources at NASA 

NASA Earth Science Data Accessibility with GIS

Airborne Geophysics

Airborne Geophysics is a method of studying the Earth's Subsurface using instruments mounted on aircraft to measure variations in Physical Properties like Magnetism, gravity, and electrical conductivity. This non-invasive technique allows for rapid and efficient data acquisition over large areas, including remote and inaccessible terrains, providing valuable information for geological mapping, mineral exploration, and environmental studies.

Airborne Electromagnetics

Airborne electromagnetics (AEM) is a geophysical surveying technique that uses electromagnetic induction to map subsurface electrical resistivity, which is related to the composition and water content of the ground. 

AEM is a rapid and efficient method for mapping Geological Structures and identifying resources like Groundwater, Minerals, and Archaeological Sites.

How Electromagnetic Works

Agricultural Remote Sensing

Advances in Remote Sensing Technology have significantly improved satellite imagery. Among the advances are improvements in Radiometric Resolution, or how sensitive an instrument is to small differences in Electromagnetic Energy. Sensors with high radiometric resolution can distinguish greater detail and variation in light.

👉 Orbits Spectrum 👉 Observing with the Electromagnetic 👉 Sensors 👉 Resolution 👉 Data Sciences 👉 Data Pathfinders

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CONTACT: peis@themughals.net

Mapping Natural Resources

Agriculture, Minerals and Groundwater

Remote Sensing can be a valuable tool in locating, mapping, and evaluating Agricultural Value Chain; Mineral Deposits and Aquifers & Groundwater.  

Spectral imaging is useful for detecting minerals in geologic formations and also for identifying minerals in sediments and accumulations of mine waste.  Remote Sensing offers the advantage of being able to evaluate large areas for mineral potential without the time and cost of on-the-ground fieldwork. Reed More....

Quantum Compatible Digital Network

Focus: Africa, Australia, Pakistan, UK & USA

Underlying Technologies

Spectral Resolution is the ability of a sensor to discern finer wavelengths, that is, having more and narrower bands. Many sensors are considered to be multispectral, meaning they have 3-10 bands. 

Some sensors have hundreds to even thousands of bands and are considered to be Hyperspectral. 

The narrower the range of wavelengths for a given band, the finer the spectral resolution. For example, the Airborne Visible/Infrared Imaging Spectrometer (AVIRIS) captures information in 224 spectral channels.  Read More....

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Group Competency

Spectrum Regulatory Compliance: NASA Science

Electromagnetic Spectrum Custom Algorithm

Pakistan Successful  Mission to Lunar South Pole

Pakistan ICUBE-Q was successfully launched on 3rd May 2024 and successfully deployed in Lunar Orbit on 8th May 2024. 

Initial images of Moon as well as Sun have been received from ICUBE-Q from the farthest point in its Elliptical Orbit.

ICUBE-Q is a CubeSat that has been designed and developed by Institute of Space Technology IST (@ISTIslamabad) in collaboration with Shanghai University SJTU.

Artemis III

NASA’s First Human Mission to Lunar South Pole

CONTEXT: The LISA (Laser Interferometer Space Antenna) Mission, led by ESA (European Space Agency) with NASA contributions, will detect Gravitational Waves in space using Three Spacecraft, separated by more than a million miles, flying in a Triangular Formation. Lasers fired between the satellites will measure how gravitational waves alter their relative distances.

On 5 April 2024, the LIGO-Virgo-KAGRA Collaboration announced the discovery of GW230529, a compact binary coalescence observed during the first part of the fourth observing run (O4a). The primary component of this binary has a mass between 2.5 and 4.5 Solar Masses. The nature of this component is uncertain as its mass is larger than the expected range for neutron stars and smaller than the expected range for black holes. The secondary component has a mass between 1.2 and 2.0 solar masses and is almost certainly a Neutron Star.

Group Advisory Services

Authentic Data from Hundreds of Earth Observation Satellites

Optical Inter-Satellite Communication System

Mapping Global Natural Resources

Agriculture - Digital Economy - Mining - Supply Chain

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DESERT HYDROLOGY

EOT LICENSING

REMOTE SENSING

Email: peis@themughals.net

Source - Reference Notes

GOV EU Remote Sensing Types Of Remote Sensing

  • Active Remote Sensing

  • "Feasibility study for a spacecraft navigation system relying on pulsar timing information" 

  • Passive Remote Sensing

  • Microwave Remote Sensing

  • The Value of Remote Sensing Data

  • Multispectral or Hyperspectral Sensors  

GOV USA DHS Mining Publication: Advances in Remote Sensing Techniques for Monitoring Rock Falls and Slope Failures

GOV USA DHS Geomagnetic Disturbance & Electromagnetic Pulse (EMP) / Geomagnetic Disturbance (GMD)

GOV USA GSA Earth Observation Technology

GOV USA Industry What is Remote Sensing? (NASA)

GOV USA Industry Digital Economy With Trusted Value Chains

GOV USA NASA APPLIED SCIENCES PROGRAM

GOV USA NASA Catalog of Earth Satellite Orbits

GOV USA NASA Remote Sensing An Overview of Satellite Remote Sensing. 

GOV USA NASA ARSET - Satellite Remote Sensing for Agricultural Applications

GOV USA NASA Remote Sensing Hyperspectral Imaging 

GOV USA NASA Remote Sensing Topographic Information for the Nation 

GOV USA NASA Remote Sensing Types Of Remote Sensing

GOV USA NASA Remote Sensing Visualization: From Energy to Image

GOV USA NASA Remote Sensing Topographic Information for the Nation 

GOV USA NIST Remote Sensing High Spectral Resolution Lidar Instrument Handbook 

GOV USA USGS Remote Sensing Aquifers & Groundwater

GOV USA USGS Remote Sensing How Do Seismometers Contribute to a Tsunami Warning System?

GOV USA USGS Remote Sensing Minerals for the Nation’s Economy

GOV USA USGS Remote Sensing Seismometers, seismographs, seismograms - what's the difference? How do they work?

GOV USA USGS Remote Sensing What is Airborne Electromagnetics?

GOV USA NASA Remote Sensing JPL Airborne Visible InfraRed Imaging Spectrometer AVIRIS 

GOV USA NOAA SPACE WEATHER CONDITIONS

YouTube Industry: Passive Microwave Remote Sensing: Applications

YouTube: Remote Sensing for Mineral Exploration

YouTube NASA: From Pixels to Products: An Overview of Satellite Remote Sensing

Additional Source Notes

▶ Al Quran: Expanding Universe 51:47

▶GOV UK BGS Earth's Magnetic Field: An Overview 

▶ Solar System Exploration Program 

▶ Electronic Countermeasures (1CM) 

▶ Electromagnetic Spectrum (EMS)  Superiority Strategy (Dr. Mark Esper) 

▶ Electromagnetic Spectrum Operations

▶ Electronic Support Measures

▶ Electronic Support Measures in Supporting Naval Operation (Indonesia Case Study)

▶ Future Weapons Technology of 2040

▶ GOV USA DOD CYBERSPACE 2019 Federal-Cybersecurity-RD-Strategic-Plan-IMP

▶ GOV USA DOD CYBERSPACE 2022 Reference and Resource Guide IMP

▶ GOV USA DOD CYBERSPACE Law Cybersecurity Enhancement Act of 2014 - S.1353

▶ GOV USA DOD CYBERSPACE STRATEGY NATIONAL 2003

▶ GOV USA DOD CYBERSPACE PROTECT THE CYBER DOMAIN

▶ GOV USA DOD CYBERSPACE STRATEGY FOR OPERATING IN CYBERSPACE

▶ GOV USA DOE: Solar Energy Basics

▶ GOV USA NASA: Earth Observation Technology Tracking Space Weather

▶ GOV USA NASA: New Study Updates NASA on Space-Based Solar Power

▶ GOV USA NASA: Orbital Collection Systems

▶ GOV USA DOE: Space-Based Solar Power

▶ GOV USA NASA: Spaceships and Rockets

▶ GOV USA NASA: Sun’s Magnetic Field

▶ GOV USA NIH: Medical Research Initiatives

▶ GOV USA WH CYBERSPACE STRATEGY 2011 INTERNATIONAL  

▶ EMS Crucial Role of Electronic Support Measures in Dominating The Spectrum

▶ EMS Invisible Battle to Jam Weapons 

▶ Key Considerations and Practical Tips to Get Published  

▶ Military Review 

▶ World Hot Spots 

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