Thank you for this great piece of equipment for flares training. It is indeed very useful. I'm learning to activate muscles I wasn't aware of. The other trainers are interested in purchasing more for our training center.
Flares... feels near impossible getting them but it's happening after 4 months of action. I'm 35 and I was giving up on this dream of mine. Thanks @gravityforcetraining for the best peace of equipment I ever used
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While the immediate focus of the group will be related to information being evaluated by the Flare Task Force, the stakeholder group will be maintained to help keep stakeholders informed and solicit comments on potential future agency actions related to flares.
A C-17A Globemaster III from Dover Air Force Base, Del., expends countermeasure flares to defeat a simulated surface-to-air missile shot from a Man-Portable Aircraft Survivability Trainer system during a training mission March 24, 2016, at the Bollen Live-Fire Range Complex on Fort Indiantown Gap, Pa. A total of 240 flares were expended from the aircraft during the training mission. (U.S. Air Force photo/Senior Airman William Johnson)
Staff Sgt. John Judy, a 436th Maintenance Squadron munitions inspector, spray paints identifying marks onto a flare stick March 28, 2016, at Dover Air Force Base, Del. All flares are assigned identifying numbers for accountability purposes. (U.S. Air Force photo/Senior Airman William Johnson)
Airman 1st Class Clay Sherrill, a 436th Maintenance Squadron munitions storage crewmember, loads a flare stick into a magazine box March 28, 2016, at Dover Air Force Base, Del. Once the magazine boxes are fully loaded, they are transported to the flightline to be uploaded onto the aircraft. (U.S. Air Force photo/Senior Airman William Johnson)
Staff Sgt. Matthew Calvo, a 736th Aircraft Maintenance Squadron communication, countermeasure and navigation system craftsman, uploads a flare magazine onto a C-17A Globemaster III on March 25, 2016, at Dover Air Force Base, Del. Each magazine consists of different flare sticks that are capable of defeating different infrared threats. (U.S. Air Force photo/Senior Airman William Johnson)
A 436th Airlift Wing C-5M Super Galaxy releases flares during a test May 12 at Eglin Air Force Base, Fla. The Dover Air Force Base aircraft and aircrew released the flares as part of a two-week defensive countermeasures test program with the 46th Test Squadron. (U.S. Air Force photo/Samuel King Jr.)
A 436th Airlift Wing C-5M Super Galaxy crosses an orange sky at sunset May 12 at Eglin Air Force Base, Fla. The Dover Air Force Base aircraft and aircrew released the flares as part of a two-week defensive countermeasures test program with the 46th Test Squadron. (U.S. Air Force photo/Samuel King Jr.)
The C-5 testing was just the start of a two-month test program. Through the end of June, the 96th Cyberspace Test Group will execute flare testing on four more aircraft from Air Force Special Operations Command, Air National Guard, Air Force Reserve Command Test Center and AMC.
Also known as the flaming rikishi, Flare Man was a top contender in the First Annual Robot Tournament due to his ferocity and size, but poor maintenance eventually cost him a chance at the finals. Though the tournament turned out to be a ploy for world domination, Flare Man did not consider himself fortunate, feeling robbed of a potentially glorious battle with the famous Mega Man. Since his creators couldn't afford to restore him to his full capacity, he was forced to take up work guarding an oil refinery deep in a remote desert. So ashamed of his loss, it is often rumored that he somehow managed to crush his own IC chip before going offline.
The MJU-73/B and MJU-62A/B infrared countermeasure flares build upon a more than 50+ year history of protecting aircrews, and will serve as an integral component of the suite of protective measures used by the military to increase aircraft survivability. Continued testing and development has enabled Northrop Grumman to deliver advanced solutions that meet the challenges posed by peer and near-peer adversaries.
Under the not-to-exceed $61.8 million IDIQ award, which has a period of performance through 2026, the company will develop cutting-edge, first-fire application technology that applies a first-fire coating to support flare ignition while increasing safety during the manufacturing process.
The purpose of this investigation was to study the influence of the flare at the lateral side of the heel of running shoes on: initial and total pronation; impact forces in heel-toe running; and to explain the results with a mechanical model. The experimental part of the study was performed by using 14 male runners. Their running movement (4 m/s) was quantified by using a force platform and high-speed film (100 frames X s-1). Three shoes were used, identical except in their lateral heel flare, one shoe with a conventional flare of 16 degrees, a second shoe with no flare, and a third shoe with a rounded heel (negative flare). The experimental results indicate that (for the used set of shoes); increasing heel flare increases the amount of initial pronation; changes in heel flare do not affect the magnitude of the total pronation; and changes in heel flare do not alter the magnitude of the impact force peaks. Since shoes with rounded lateral heels do reduce initial pronation, it is speculated that this construction could be used to prevent anterior medial compartment syndrome at the tibia of runners. It was concluded that more research is needed to specify whether the reported result is representative for various shoe types or is shoe specific.
The white flare of the Force was one of the equal and balanced parts of the Force that comprised all worlds. The white flare's heat and intensity differed from but was in harmony with the black current of the Force. The flare was a brightness in beings who were Force-sensitive. Its searing torrent rose like a bonfire that could be a steady beacon or become a blast or an explosion.[1]
The white flare of the Force was first depicted in "The Duel," a short film in the Star Wars: Visions series produced by Kamikaze Douga and directed by Takanobu Mizuno,[3] and first identified in the tie-in novel Ronin: A Visions Novel, written by Emma Mieko Candon.[1] Instead of a light side and dark side of the Force, Candon drew upon the concepts of Taoism and yin/yang as part of re-envisioning the Force as closer to its Japanese cultural inspirations. The white flare is therefore neither light nor dark side.[2]
During eruptive flares, vector magnetograms show an increasing horizontal magnetic field and downward Lorentz force in the Sun's photosphere around the polarity-inversion line (PIL). This behavior has often been associated with the implosion conjecture and has been interpreted as the result of either momentum conservation while the eruption moves upward or of the contraction of flare loops. We characterize the physical origin of these observed behaviors by analyzing a generic 3D magnetohydrodynamics simulation of an eruptive flare. Even though the simulation was not designed to recover the magnetic field and Lorentz force properties, it is fully consistent with them, and it provides key additional information for understanding them. The area where the magnetic field increases gradually develops between current ribbons, which spread away from each other and are connected to the coronal region. This area is merely the footprint of the coronal post-flare loops, whose contraction increases their shear field component and the magnetic energy density, in line with the ideal induction equation. For simulated data, we computed the Lorentz force density map by applying the method used in observations. We obtained an increase in the downward component of the Lorentz force density around the PIL, consistent with observations. However, this significantly differs from the Lorentz force density maps that are obtained directly from the 3D magnetic field and current. These results altogether question previous interpretations that were based on the implosion conjecture and momentum conservation with the coronal mass ejection, and rather imply that the observed increases in photospheric horizontal magnetic fields result from the reconnection-driven contraction of sheared flare loops. be457b7860
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