Download Dark Conversation By Rod Wave ((FULL))

In the chorus, he speaks of having conversations in the dark, implying that he often engages in self-reflective moments when he is alone. During these moments, he confronts his own fears, insecurities, and the weight that his heart carries. He acknowledges that his heart has been hurt before and pleads for it not to be hurt again. This represents a desire to protect oneself from further pain and disappointment.

Despite these dark thoughts, he finds moments of solace and motivation to keep going. The mention of Reginae and Charmaine, presumably loved ones or sources of inspiration, reminds him of the reasons why he should continue living. Though he may feel alone at times, he seeks refuge in his own company, creating a zone where he can process his thoughts and emotions.

Download Dark Conversation By Rod Wave

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My friends call me froth queen; I surf every morning at dark o'clock whether it's too flat, big, cold, or windy because that's my only me time. I am a full-time mother to a wild toddler, and in the spaces in between, I make illustrations and work on my labor of love, Sunday Arvo Surf Club.

I traveled around the world for a few years living out of a suitcase, learning about myself, and learning how to surf. I lived lightly, spent much less money than I would have than if I were home, and was the happiest I'd ever been. I constantly remind myself of that time and try to remember you don't need much for happiness and to live simply. Money, jobs, careers, and material things come and go. What matters is living a life you love being full of love, and being kind to others. There are so many moments that I hold dear in my heart from a stranger that has saved me from a dark time.

Unlike light waves, gravitational waves are nearly unimpeded by the galaxies, stars, gas and dust that fill the universe. This means that by measuring gravitational waves, astrophysicists like me can peek directly into the heart of some of these most spectacular phenomena in the universe.

By detecting more events that create gravitational waves, there will be more opportunities for astronomers to also observe the light produced by those same events. Seeing an event through multiple channels of information, an approach called multi-messenger astronomy, provides astronomers rare and coveted opportunities to learn about physics far beyond the realm of any laboratory testing.

Gravitational waves are created when massive objects like black holes or neutron stars merge with one another, producing sudden, large changes in space. The process of space warping and flexing sends ripples across the universe like a wave across a still pond. These waves travel out in all directions from a disturbance, minutely bending space as they do so and ever so slightly changing the distance between objects in their way.

Even though the astronomical events that produce gravitational waves involve some of the most massive objects in the universe, the stretching and contracting of space is infinitesimally small. A strong gravitational wave passing through the Milky Way may only change the diameter of the entire galaxy by three feet (one meter).

To measure gravitational waves, researchers shine a laser from the center of the facility to the base of the L. There, the laser is split so that a beam travels down each arm, reflects off a mirror and returns to the base. If a gravitational wave passes through the arms while the laser is shining, the two beams will return to the center at ever so slightly different times. By measuring this difference, physicists can discern that a gravitational wave passed through the facility.

LIGO began operating in the early 2000s, but it was not sensitive enough to detect gravitational waves. So, in 2010, the LIGO team temporarily shut down the facility to perform upgrades to boost sensitivity. The upgraded version of LIGO started collecting data in 2015 and almost immediately detected gravitational waves produced from the merger of two black holes.

Between each run, scientists improved the physical components of the detectors and data analysis methods. By the end of run O3 in March 2020, researchers in the LIGO and Virgo collaboration had detected about 90 gravitational waves from the merging of black holes and neutron stars.

Scientists have been working on many technological improvements. One particularly promising upgrade involved adding a 1,000-foot (300-meter) optical cavity to improve a technique called squeezing. Squeezing allows scientists to reduce detector noise using the quantum properties of light. With this upgrade, the LIGO team should be able to detect much weaker gravitational waves than before.

My teammates and I are data scientists in the LIGO collaboration, and we have been working on a number of different upgrades to software used to process LIGO data and the algorithms that recognize signs of gravitational waves in that data. These algorithms function by searching for patterns that match theoretical models of millions of possible black hole and neutron star merger events. The improved algorithm should be able to more easily pick out the faint signs of gravitational waves from background noise in the data than the previous versions of the algorithms.

Astronomers have captured both the gravitational waves and light produced by a single event, the merger of two neutron stars. The change in light can be seen over the course of a few days in the top right inset.

Hubble Space Telescope, NASA and ESA

LAB: Perhaps my interest in the ocean is rooted in the fact that I grew up in Mazatln, a coastal town (now a city) in the state of Sinaloa. Every day we woke up to the ocean, and the beach was where my sisters and I would play and explore for hours after school. We had no interest in toys; the beach and the ocean had everything: it is a place of marvel, a place that is different every day; it is teeming with life on the surface, in the sand, and in the water; sunsets are spectacular and different every day, with millions of colors painting the sky. It is a place of delight as well as of mystery. And as children, it was not unusual for us to be woken up in the middle of the night by a loudspeaker telling us to evacuate the area because of the possible dangers of an approaching ola marina [tidal wave or hurricane]. We were continually reminded of the powerful presence of nature, and of the importance of listening to it, respecting it, and getting out of its way when necessary. Nature was just part of life.

Now, at the start of the second decade of the twenty-first century, I look back on the progress spurred in 1992, which marked an important shift in global policy and social consciousness in terms of the protection of our environment and the communities that live in close relationship with it. However, these gains stand at risk of being systematically erased and replaced with shortsighted agendas that serve the privileged few. To feel discouraged by this reality only paralyzes us. We have the opportunity to make an impact, beginning by recognizing that our personal choices have tremendous power. We can inspire others to take a stance and to change the values and practices of private industry and policy. We are at a crossroads. I created Intervention: Ocean Calling and Ocean Blues in response to these issues, and although these works in themselves will not solve the problems we are facing, they can inspire necessary conversations, and ultimately, ideally, make some waves.

For centuries, humans have explored the Universe and discovered novel astrophysical sources and phenomena only through the observation of electromagnetic waves (gamma rays, X-rays, optical, infrared, radio waves). In 2015, we observed the first gravitational wave passing through the Earth produced by the merger of two stellar-mass black holes. Such an event has provided us with a remarkable confirmation of the general theory of relativity by Albert Einstein, and ushered in the era of gravitational-wave astronomy. Since then, about 100 gravitational waves have been detected, including the gravitational signal produced by the coalescence of two neutron stars, accompanied by a plethora of electromagnetic counterparts observed by numerous telescopes around the world.

The 2023 release wave 2 plan covers all new functionalities planned to be delivered to market from October 2023 to March 2024. In this article, you'll find the product overview and what's new and planned for Dynamics 365 Customer Service.

Copilot and AI innovationCopilot transforms the Customer Service support experience with generative AI. Copilot helps agents easily use internal knowledge sources by generating optimized responses in a single click. Agents are more productive and deliver better service experience with Copilot helping them find resources to resolve issues faster, handle cases more efficiently, and automate time-consuming tasks. To name a few features, Copilot drafts contextual answers to questions in chat and email, responds to questions from the agent, and generates case and conversation summaries.

OmnichannelThe omnichannel capabilities in Dynamics 365 Customer Service enable organizations to instantly connect and engage with their customers via channels like live chat, SMS, voice, Microsoft Teams, and social channels. By providing a seamless agent experience and valuable conversation insights across channels, the omnichannel features enable organizations to deliver a true, all-in-one contact center.

Features that must be enabled by application administrators

This release wave contains features that must be enabled or configured by administrators, makers, or business analysts to be available for their users. For the complete list, look for all features tagged "Users by admins, makers, or analysts" in the release plan.

When black holes and other enormously massive, dense objects whirl around one another, they send out ripples in space and time called gravitational waves. These waves are one of the few ways we have to study the enigmatic cosmic giants that create them. ff782bc1db