https://www.youtube.com/watch?v=IozXyOBbUWE
Part 2 of a lesson on basic counter surveillance.

https://www.facebook.com/IssTrainingLtd/videos/2-basic-counter-surveillance-tutorial-pt-2/1036484840188934/
Part 2 of our basic counter surveillance lesson.

https://protectioncircle.org/2015/04/17/surveillance-surveillance-detection-and-counter-surveillance/
Counter Surveillance (CS) Counter surveillance is a follow-up measure that is taken only after hostile surveillance has been detected. CS basically turns the tables by conducting surveillance on the surveillance in order to collect more detailed information on it. It must therefore be conducted in at least as covert a manner as SD, if not more

https://www.reddit.com/r/Gangstalking/comments/18eog6h/counter_surveillance_pt_2/
The Forever Chemical Scandal (2023) PFAS chemicals are used in thousands of products aimed at making life easier. But the chemicals are now almost everywhere, including in human blood, and are being linked to severe health problems. [00:48:02]

https://www.itstactical.com/intellicom/physical-security/psd-concepts-how-to-detect-surveillance-and-counter/
Surveillance continues as the attack is planned and practiced. Attackers deploy according to the information received. Surveillance is also used to confirm your arrival immediately prior to an attack. Once the attack has begun the attackers have a huge advantage. They have set the time and place that you are the most vulnerable and most exposed.

https://circuit-magazine.com/counter-surveillance/
Counter Surveillance is a complex subject and is frequently neglected on CP courses and often misunderstood. Therefore, in the space available here, I'm going to point out the key principles to a counter surveillance operation. Counter Surveillance is defined as the actions that a person (or team) carries out, in order to detect that a person (Principal) is under surveillance and to identify

https://www.collinsaerospace.com/what-we-do/industries/commercial-aviation/flight-deck/surveillance/integrated-surveillance/iss-2100-configurable-integrated-surveillance-system
The ISS-2100 configurable integrated surveillance system simplifies surveillance by joining several features - such as weather detection, traffic alert and collision avoidance, Mode S surveillance and terrain awareness and warning functions - into a single system. The ISS-2100 significantly enhances the safety of your flights, lowers

https://read.circuit-magazine.com/articles/article-128936
Counter Surveillance By: Peter Jenkins, ISS Training LTD Peter Jenkins has worked internationally with CP Teams in a CS role and this article is an extract from the chapter on surveillance detection in his forthcoming book The Theory of Covert Surveillance. The post The Key Elements of Counter Surveillance appeared first on Circuit Magazine.

https://www.intelsecurity.co.uk/courses?view=courses&task=course&category=3&course=93
What the Students Can Expect. This three day course teaches the skill sets required to operate as a sophisticated counter surveillance team. In order to fully appreciate 'what to look for' it also teaches the basic understanding of how a surveillance team operates. Students completing this course receive a certificate of completion.

https://www.issnationallab.org/117-billion-particles-and-counting/
AMS-02 was launched to the ISS on the Space Shuttle Endeavour in May 2011 and has measured more than 117 billion particles to date! Learn more about AMS-02 and other ISS National Lab projects looking outward into space in the Upward feature, " On the Frontier of Space: Looking Outward to Better Understand the Universe Around Us ."

https://satelliteobservation.net/2018/03/08/contested-space-ii-countermeasures/
Detecting the engagement. As seen in Contested Space I: Threats , the terminal guidance of ASAT systems can be either infrared or radar, so countermeasures against both are required. However, a first step before activating countermeasures it to realize that they are needed, by detecting the engagement has taken place.

https://www.sciencedirect.com/science/article/pii/S0168900212004974
The AMS-02 detector is a large acceptance particle spectrometer (0.5 m 2 sr). A schematic view of the final layout of the detector is shown in Fig. 1.It consists of a transition radiation detector (TRD), a time-of-flight system (TOF), a permanent magnet (PM), a precision silicon strip tracker, an anti-coincidence counter system (ACC) surrounding the inner tracker, a Ring Image Cherenkov

https://www.sciencedirect.com/science/article/pii/S0168900212005682
Fig. 1. The AMS-02 spectrometer, which is made of Transition Radiation Detector (TRD), Time-of-flight (TOF) hodoscopes, Silicon Tracker, Veto or anti coincidence counters (ACC), Ring Imaging Cherenkov counter (RICH), and sampling calorimeter (ECAL). The AMS-02 spectrometer operates on the ISS at an altitude of 400 km, free from backgrounds of

https://ams02.space/
A state-of-the-art particle detector installed on the International Space Station. Discover AMS. Integration of AMS. AMS to be launched. AMS installed on the ISS. AMS on orbit. ... Anti-Coincidence Counter. Ring Imaging Cherenkov Detector. Electromagnetic Calorimeter. ... AMS-02 time on ISS since May 19th, 5:46 a.m. EDT: 00. Days. 00. Hours. 00

https://ams02.space/detector
AMS is a TeV precision, multipurpose particle physics magnetic spectrometer. It identifies particles and nuclei by their charge (Z), energy (E) and momentum (P), which are measured independently by the Tracker, TOF, RICH and ECAL. The ACC counters (not shown in the Figure) are located in the magnet bore. As seen in Figure 1, the AMS detector

https://www.sciencedirect.com/science/article/abs/pii/S0168900212005682
The Alpha Magnetic Spectrometer (AMS-02) is a large acceptance cosmic-ray detector which has been installed as an independent module on the International Space Station (ISS) in May/2011 after the successful launch of STS-134. The instrument will provide a precise measurement of the cosmic-ray energy spectra and extensive antimatter search up to 1 ∼ 2 TeV for particle charges up to Z=26.

https://militaryyearbookproject.org/references/military-occupation-codes/usmc/field-02-intelligence/mos-0212-technical-surveillance-countermeasures-specialist
This MOS is to be assigned only as a NMOS and will be assigned and voided only by the. authority of the CMC (MM). Prerequisites. (1) Must hold primary MOS 0211, 2621, 2631, or 2651. (2) Must be a sergeant or above. (3) Prior to entry into the TSCM Course, must have sufficient obligated service to allow 36 months remaining upon graduation.

https://iopscience.iop.org/article/10.1088/1742-6596/2429/1/012002
The Alpha Magnetic Spectrometer, AMS-02, is a magnetic spectrometer detector operating on the International Space Station (ISS) since May the 19 th, 2011.More than 200 billion events have been collected by the instrument in the first 11 years of data taking, providing detailed and novel insights on the composition and energy spectra of cosmic rays up to TeV energies.

https://www.esa.int/ESA_Multimedia/Images/2019/11/AMS-02_on_the_International_Space_Station
AMS-02 on the International Space Station. 08/11/2019 1345 views 7 likes 433362 ID. Like. Download. HI-RES JPG [283.81 kB] ... the AMS-02, is mounted on the upper Payload Attach Point on the S3 Truss of the International Space Station (ISS). CREDIT AMS-02 LICENCE ESA Standard Licence; Human Spaceflight. Beyond. Science & Exploration Soyuz MS-13

https://s3.cern.ch/inspire-prod-files-b/b6192da652a3e0eb93342f2db6a8e7c6
The Alpha Magnetic Spectrometer (AMS-02) on the International Space Station (ISS) is a large acceptance magnetic spectrometer aiming for high precision studies of cosmic rays in space. The experiment will address fundamental questions regarding primary antimatter and ... counter (RICH) and the electromag-netic calorimeter (ECAL) are shown. The

https://www.epj-conferences.org/articles/epjconf/pdf/2019/14/epjconf_ricap2019_01014.pdf
The Alpha Magnetic Spectrometer, AMS-02, is a general purpose high energy particle physics de-tector. It was launched to space with the Space Shuttle STS-134 mission and installed onboard the ISS in 2011, on May 19th, to conduct a unique long duration mission (up to the lifetime of the ISS) of fundamental physics research in space.

https://www.peraton.com/capabilities/operations/c2-isr/
We deliver an integrated set of Space Awareness, C2, Mission Applications and Infrastructure to enable multi-domain operations. We provide integrated transport services for ISR airborne and spaceborne systems, as well as vehicle and sensor payload planning. Full Lifecycle C2 & ISR. Mission Management. Mission Planning.

https://galprop.stanford.edu/elibrary/icrc/2009/preliminary/pdf/icrc1273.pdf
AMS-02 is a large acceptance (∼ 0.5 m2sr) magnetic spectrometer designed to measure the cosmic rays fluxes in the rigidity range from 0.5 GV to 4 TV. The AMS-02 launch on the Space Shuttle is scheduled for September 2010 and the detector is now in its final integration phase at CERN. After a beam test, to be performed in fall 2009 at CERN