eyes-on-exoplanets

High Precision Laser Fault Injection using Low-cost Components

High Precision Laser Fault Injection using Low-cost Components.

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 // Unprotected var Flag = FALSE func test() ... if (Flag == TRUE) return SecretOp() else return EXPECTED end func SecretOp() ... return SECRET end

// Double Test ... if (Flag == TRUE) if (Flag == TRUE) return SecretOp() else TRAPPED else return EXPECTED

 // Retest in Target func SecretOp() if (Flag == TRUE) ... return SECRET else TRAPPED end

// Inverse Test ... if (Flag == TRUE) if (Flag != TRUE) TRAPPED else return SecretOp() else return EXPECTED

 // Double Data ... if ((FlagA == FALSE) && (FlagB == FALSE)) return EXPECTED elseif ((FlagA == TRUE) && (FlagB == TRUE)) return SecretOp() else TRAPPED

// Inverse data ... if (Flag != ~InvFlag) TRAPPED elseif (Flag == TRUE) return SecretOp() elseif (Flag == FALSE) return EXPECTED else TRAPPED

 // Checksum over data ... CrcVerify_TrapOnError() ... if (Flag == TRUE) return SecretOp() else return EXPECTED

// Redundant Representation const STRUE = 0xA5 const SFALSE = 0xA7 ... if (Flag == STRUE) return SecretOp() elseif (Flag == SFALSE) return EXPECTED else TRAPPED

 // Repeated Calculation ... u16 nTmp1 = SecretOp() u16 nTmp2 = SecretOp() if (nTmp1 != nTmp2) TRAPPED else return nTmp2;

// Modified & Compensated ... Tmp1 = Calculation(Rnd1) Tmp2 = Calculation(Rnd2) Tmp3 = Clear(Tmp1, Rnd1) Tmp4 = Clear(Tmp2, Rnd2) if (Tmp3 != Tmp4) TRAPPED else return Tmp3

 // Alternative Algorithm ... Tmp1 = Method1() Tmp2 = Method2() if (Tmp1 != Tmp) TRAPPED else return Tmp2

// Inverse Calculation ... Tmp1 = Method(Input) Tmp2 = InvMethod(Tmp1) if (Input != Tmp2) TRAPPED else return Tmp1

// Jump ID func ProtectedFn() if (!IdVerify(CALL_F)) TRAPPED else ... IdSet(RET_F) return Result end ... IdSet(CALL_F) Val = ProtectedFn() if (IdVerify(RET_F)) TRAPPED else return Val

 // Waymark - Late Test WM = IV ... WM += M1 ... WM += Mx ... if (WM != IV+M1+...Mx) TRAPPED else return nRetVal

// Waymark - On the fly func Waymark(n) if (n != nNextWM) TRAPPED else nNextWM++ end ... Waymark(10) ... Waymark(11) ... Waymark(12) return Result

-------------------------------------

// Hybrid Defense func Calculation(WP) Waymark(WP) ... Waymark(WP+1) return EXPECTED func TestEQ(WP, V1, V2) Waymark(WP) return (V1 == V2) ... A = Calculation(1) B = Calculation(3) if (TestEQ(5, A, B)) if (TestEQ(6, B, A)) Waymark(7) return A TRAPPED

https://pure.royalholloway.ac.uk/ws/files/38226452/00_AfforableLaserAttacks.pdf

https://drive.google.com/file/d/1c218i0LF0bRlonn12TD0wcDzM8z9I3-m/view?usp=sharing

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handheld/drone package and satellite incoming:

RAM OS takeover and firmware reflashing for military device takeover 

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https://barleysarthistory.blogspot.com/2024/09/remote-control-of-enemy-systems.html

https://barleysarthistory.blogspot.com/2024/08/block-chain-technology-government.html

Remote adjustment utilizing existing infrastructure


Mars Perseverance Sol 1314: Left Navigation Camera (Navcam) gif

 dust devil near center



Mars Perseverance Sol 1314: Left Navigation Camera (Navcam) gif

NASA's Mars Perseverance rover acquired these images using its onboard Left Navigation Camera (Navcam). The camera is located high on the rover's mast and aids in driving.

Images acquired on Oct. 30, 2024 (Sol 1314) at the local mean solar time of 14:52:39 to 14:54:26.

Image Credit: NASA/JPL-Caltech

Assembled by Barley Culiner with GIMP

We Fell For The Oldest Lie On The Internet


9,000 to 19,000 km length for all the blood vessels in a human
not 100,000 km

We Fell For The Oldest Lie On The Internet

Report on the Historical Record of U.S. Government Involvement with Unidentified Anomalous Phenomena (UAP)

THE DEPARTMENT OF DEFENSE

ALL-DOMAIN ANOMALY RESOLUTION OFFICE

Report on the Historical Record of U.S. Government Involvement

with Unidentified Anomalous Phenomena (UAP)

Volume I

February 2024

https://media.defense.gov/2024/Mar/08/2003409233/-1/-1/0/DOPSR-CLEARED-508-COMPLIANT-HRRV1-08-MAR-2024-FINAL.PDF


OFFICE OF THE DIRECTOR OF NATIONAL INTELLIGENCE

Preliminary Assessment:

Unidentified Aerial Phenomena

https://www.dni.gov/files/ODNI/documents/assessments/Prelimary-Assessment-UAP-20210625.pdf




67P/Churyumov–Gerasimenko

 














67P/Churyumov–Gerasimenko

https://www.esa.int/Science_Exploration/Space_Science/Rosetta

https://sci.esa.int/web/rosetta/-/14615-comet-67p

Assembled by Barley Culiner with GIMP

ROSETTA

MISSIONHOSTINSTRUMENTPRINCIPAL INVESTIGATOR(S)
RosettaOrbiterALICES. A. Stern (SwRI, Boulder, USA)
  CONSERTW. Kofman (LPG, Grenoble, France)
  COSIMAM. Hilchenbach (MPS, Katlenburg-Lindau, Germany)
  GIADAA. Rotundi (Università degli studi di Napoli “Parthenope”)
  MIDASM. Bentley (IWF, Graz, Austria)
  MIROM. Hofstadter (NASA/JPL, Pasadena, USA)
  NAVCAMThe NAVCAM is commanded by the Rosetta Flight Dynamics and Flight Control Teams at ESOC. The data were processed and archived by the Rosetta Science Ground Segment (SGS) and the Planetary Science Archive Team (PSA) at ESAC.
  OSIRISH. Sierks (MPS, Goettingen, Germany)
  ROSINAK. Altwegg (University of Bern, Switzerland)
  RPCICAH. Nilsson (Swedish Institute of Space Physics, Kiruna, Sweden)
  RPCIESJ. Burch (SwRI, San Antonio, TX., USA)
  RPCLAPA. Eriksson (Swedish Institute of Space Physics, Uppsala, Sweden)
  RPCMAGK-H Glassmeier (TU Braunschweig, Germany)
  RPCMIPP. Henri (LPC2E/CNRS, Orléans, France)
  RSIM. Paetzold (University of Cologne, Cologne, Germany)
  VIRTISF. Capaccioni (IAPS-INAF, Rome, Italy)
 Philae LanderAPXSG. Klingenhoefer (Gutenberg-University, Mainz, Germany)
  CIVAJ.P. Bibring (Institut d'Astrophysique Spatiale, France)
  CONSERTW. Kofman (LPG, Grenoble, France)
  COSACF. Goesmann (MPS, Goettingen, Germany)
  MUPUST. Spohn (DLR, Germany)
  PTOLEMYI. Wright (Open University, UK)
  ROLISS. Mottola (DLR, Germany)
  ROMAPH-U. Auster (Technische Universitaet Braunschweig, Germany)
  SD2A. Ercoli-Finzi, (Politecnico di Milano, Italy)
  SESAME

M. Knapmeyer (DLR, Germany)

 AncillaryShape ModelThe shape models have been produced using data from the OSIRIS and NAVCAM instruments. Consult the CITATION_DESC in the label of each product you use and make sure that you cite / acknowledge the relevant data producer listed there.

Mars Perseverance Sol 1303: Right Mastcam-Z Camera stitch

 

Mars Perseverance Sol 1303: Right Mastcam-Z Camera stitch

NASA's Mars Perseverance rover acquired these images using its Right Mastcam-Z camera. Mastcam-Z is a pair of cameras located high on the rover's mast.

Images acquired on Oct. 19, 2024 (Sol 1303) at the local mean solar time of 12:54:00 to 12:56:37.

Image Credit: NASA/JPL-Caltech/ASU

Assembled by Barley Culiner with Microsoft ICE

Mars Perseverance Sol 1303: Right Mastcam-Z Camera stitch

NASA's Mars Perseverance rover acquired these images using its Right Mastcam-Z camera. Mastcam-Z is a pair of cameras located high on the rover's mast.

Images acquired on Oct. 19, 2024 (Sol 1303) at the local mean solar time of 12:56:52 to 13:00:57.

Image Credit: NASA/JPL-Caltech/ASU

Assembled by Barley Culiner with Microsoft ICE

Additional editing with GIMP

Mars Perseverance Sol 1299: Right Mastcam-Z Camera stitch

Mars Perseverance Sol 1299: Right Mastcam-Z Camera stitch

NASA's Mars Perseverance rover acquired these images using its Right Mastcam-Z camera. Mastcam-Z is a pair of cameras located high on the rover's mast.

Images acquired on Oct. 15, 2024 (Sol 1299) at the local mean solar time of 12:46:35 to 12:55:28.

Image Credit: NASA/JPL-Caltech/ASU

Assembled by Barley Culiner with Microsoft ICE

Additional editing with GIMP

full size image:

https://www.gigapan.org/gigapans/236138

Mars Perseverance Sol 1299: Left Navigation Camera (Navcam) gif

 dust devil near center left

Mars Perseverance Sol 1299: Left Navigation Camera (Navcam) gif

NASA's Mars Perseverance rover acquired these images using its onboard Left Navigation Camera (Navcam). The camera is located high on the rover's mast and aids in driving.

Images acquired on Oct. 15, 2024 (Sol 1299) at the local mean solar time of 13:02:48 to 13:04:09.

Image Credit: NASA/JPL-Caltech

Assembled by Barley Culiner with GIMP

Disassemble Mercury in order to construct Dyson swarm

Disassemble Mercury in order to construct Dyson swarm

from

Gezeichnet Dan Gallagher (KBR Wyle Services, LLC)
to

Gezeichnet Karl Bednarik

Gemini & Barley:

if we disassembled Mercury to create a Dyson swarm would the rotation of the inner planets change

Disassembling Mercury to create a Dyson swarm would likely have a negligible effect on the rotation of the inner planets.

Here's why:

Mercury's small mass: Compared to the other planets, especially the gas giants, Mercury's mass is relatively insignificant. Its gravitational influence on the other planets is minimal.

Dyson swarm's distribution: A Dyson swarm would be distributed around the star, creating a relatively symmetrical mass distribution. This would minimize any gravitational perturbations on the inner planets.

Orbital mechanics: The orbits of the inner planets are primarily determined by the Sun's gravity. The removal of Mercury's mass would not significantly alter this balance.

While there might be some minor adjustments due to gravitational interactions, the overall stability of the inner planets' orbits would likely remain largely unaffected.

orient satellite swarm to reduce the effects of climate change

collect solar energy and utilize power beaming technology

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Robotic swarm technology for rapid Mercury satellite construction factories

Mesh data and power beaming network required for Dyson swarm

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Viability of a Dyson Swarm as a Form of Dyson Sphere https://arxiv.org/abs/2109.11443

Power beaming comes of age https://www.technologyreview.com/2022/10/06/1060650/power-beaming-comes-of-age/

Researchers Enlist Robot Swarms to Mine Lunar Resources https://news.arizona.edu/news/researchers-enlist-robot-swarms-mine-lunar-resources

Autonomous Robot Swarms for Lunar Orbit Servicing and Space Asset Assembly https://techport.nasa.gov/view/106703