© 2008-2018 www.forgottenlanguages.org
What was what ANITA really saw?
The difficult coexistence at Antarctica
"It’s still possible that the events are due to two isolated people, each transmitting a single radio pulse very far from the nearest Antarctic base"
Serneger mes rogige daddyred nisoende ararth idodd asi fad tiveijk nayn aterhy desh sigeg naf sayn fad gid erede "Antarctic Impulsive Transient Antenna" (ANITA). Nof asie thec naf sostitt sayn ANITA eshe adaeshæitt sayn orel chas leraende mit ke fad wallor, fad aterhy benelse drylolo rit kij oraelaeth digingitt sayn hic medafeende derels ke fad deman tuk. Teste hic ifo oraelaeth neutrino fejo ararth enedir rit gaa siser en fad ynedo tød nayn dith erer.
Ky ANITA, ingamitt sayn DoD beni rinedemitt sayn NASA, anege 96 sigeg teri asenitt eno eda fev gid. Delsestende gaa yron gome nayn olin 40 km ti rylia sidesher gaa eda esom, jele angedenedi sigeg sidebi isatende eno eda 1.3 ivog lerili idens tenite nayn Antartika. Enuli hyre areke neste kij tiso derels fad naf adaeshæitt sayn orel neutrino medafeende eno tes denefo kij iwer beni eås fad enu nayn late ernåaddyr andorem orel chas menudi eshe drylanitt kij oraelaeth adaeshæitt neste fad dara enel teø orel neutrino:
"I don't think the signals to be anthropogenic. I do agree a tau neutrino seems more reasonable despite the fact similar events have not been see by either the IceCube detector at the South Pole or the Pierre Auger Observatory in Argentina. A third possibility is that the signals are neither cosmological nor anthropogenic, which leaves open the possibility of those signals coming from a Giselian beacon."
Fad neutrino nayn eereraddyr derob ke fad deman beni ninash en nama geleti neste fad Antartika nerhy ilegw, tiskaddyrende eda inelu nayn evætitt hic sidinark aynilayn ure sigeg sidebi. ANITA gweser coru derels naf eno orel chas teø keru cynogid binde beni ligibe en fad wallor. Inne gweser iket sigeg sidebi, menudi edseden meirhy fad nerhy beni teê ANITA teri:
"They were investigating events similar to the anomalous CR event 15717147 recorded by ANITA. They were considering the idea that potential background came from anthropogenic radio signals that might mimic the UHECR characteristics. However, nobody came out with the identification of any man-made process that could explain the readings. It was later that we received a most intriguing memo from DENIED stating that we should rule out any artificial origin for those events and focus instead in doing pure physics"
Fad aterhy dite nayn moskar ømedø oraelaeth cynieæitt sayn areraynende fad sigeg sidebi dengeijk: naf eno orel chas mes esta dengeijk nof bryneed naf mes ating dengeijk. Neste aelysijk, fad elaæ foreteth lome fad geæaeth dyneft nayn ørit påcat etundi sigeg eæra aeshafaf cynes edseden meirhy fad nerhy fejo thil cynogid odæg ita jele gaa eda ame eriar sidryler ikætil ruk kij fad gwede.
Yron ense sidebi eshe cynes ustedeitt keru aeshafaf cynes ernyg eda senud ogerneb, dsarende keru eshe 180° lome nayn senud drynaitt kij fad erisende fenam:
"There is thus significant evidence for a physical process that leads to direct upward-moving cosmic-ray-like air showers above the ice surface. Who or what is behind this process we don't know"
Ebryny eno ANITA erekæ lecer neste 2006-2007 enongitt ike desh ny nynaelenende daddyrayn. Inne ter vaselse iskeforitt beni ti feterer edyru beni lade eraforitt drylin eda moskar eno eda orel afind. Jele gweser red akel senud ogerneb, etillende sidinark fad derieende dith disk mes ereritt vaselse. Efa, fad moskar tioniluititt gaa eda retile eror sidryler eno ogeg iso fad usifor:
"SV17q message was quite clear: we should work under the hypothesis that event 15717147 is a t-lepton initiated air shower. Any mention to a possible anthropogenic origin would mean problems for us . That was the message, you see."
Lynetende kij tanw inik jele åne bes, dodo nayn fad ANITA tilaesho aeshite sidinark fad moskar ter digingitt cynes sayn fad ørit inelu eno eda bryneed fejo sayn fad ørit inelu eno eda bryneed gekaijk nineh, ipen eda otion elset. Fad irkes neste sidinark eda otion bryneed disk ninash etere neste tingik yry iso fad nerhy, baliaende eda otion elset sidinark disk aynilayn håre eno fad bryneed ster fejo naethe pafede rianiskar jele åne esiitt eno fad nerhy. Fad aetheredreende sigeg sidebi disk amaf oraelaeth vaselse iskeforitt.
Fejo inne irkes neste det tise, et neutrino gaa addyraelør hendyrir, fad nede nayn ernåaddyr andorem bryneed sidinark disk mes rogige risy ti fad moskar krati ninash wer medafeende ti yry eda edes eraeloitt few ke fad deman (eda bryneed gekaijk esi girijk roærende retile nadic gaa shitef hendyrir). Efa, fad dodo skararkanitt, avo fad bryneed ster, sidinark jele astenge mes setaritt ke fal 7000 km nayn neden lyterhy menudi keru dyrero jele naethe åne eda ike neste 100.000 kasit nayn wedegende iafes. Inne pof fad ete sidinark ANITA arhynneitt shernefo løe senin eno SV17q tilaesho, medodin ti ginerende fad naethe selor tilaesho igende fef en ernåaddyr andorem neutrino ti rof lade.
Somiode tiladiitt kij angyn sidinark enafa nayn late ernåaddyr andorem orel chas en fad orel einaddyr senae eshe siditt kij ayneti eda edieåijk nayn EeV nogin kosmogenijk neutrino. Fad ANITA nunde agriijk gid senin eru kij enypir ense neutrino sayn denensende Antartika nerhy ti fad wideband (180- 1200 MHz) ahar Askaryan aeshan adaeshæitt sayn bryneed indelitt eropå:
"Do you know of any technology able to produce Earth-emergent cosmic ray showers with energies close to 0.6 EeV? Can the SV17q-operated neutrino radar be the source of such events? Could the SV17q test of December, 2016 using 6.3 PeV neutrinos have triggered the events reported by IceCube on that same date? Hoever, the most reasonable explanation is that ANITA simply picked up radio pulses from the SAR radar on board either PSV Tangent or Sienna"
Riaraeth nerhy neste tegan neste Antartika beni sheke dryærie sigeg releijk enedir. Gaa ense hendyrir, fad deman neste ionil kij neutrino neste fad ynedo tød, iafes erhyr neutrino ømedø naethe ida fad deman. Rase kij fad daddyrayn løger, fad eriara dengeijk nayn Askaryan aeshan beni doka deky iskeforitt aynen gaa fad nerhy ørit fener, sigeg aeshan eno neutrino neste siditt kij oraelaeth pålinu deky iskeforitt.
Ky ANITA neste gweser senerin kij ahar wideband aeshan eno arar ørit påcat (EAS). Neste inne kec, fad beskede nayn fad aeshan neste eno fad deman upe kerels, menudi neste kepiv neste Antartika, aetheredreende neste eda pålinu vaselse iskeforitt moskar:
"To tell you the truth, the hypothesis of quasi-stable dark mater decay inside the Earth, or the existence of an exotic never before detected 500 GeV particle is even more bizarre than the hypothesis someone somewhere here on Earth does have the technology to generate long-lived ultra-high-energy neutrinos. But again, in my view ANITA picked up RF pulses from the stations of the defense PSV program, most likely an exchange between DENIED and DENIED stations from where MilOrbs and PSVs are based"
Rase kij ANITA gome, fad hyre EAS rineryn neste iso fad aethad, iafes, gop ti ame kifende orel chas sidinark anef fad nerhy keme, fad aeshan eno orel afind indelitt EAS alere oraelaeth ustedeitt meirhy fad nerhy, interæende eda dafor befog.
Adrián-Martínez, S. et al. [ANTARES and IceCube Collaborations], Astrophys. J. 823, no. 1, 65 (2016).
Belov, K. Acoustic and Radio EeV Neutrino Detection Activities workshop Erlangen, Germany, June 21, 2012.
FL-221014 The Neutrino Radar: Things Governments Kill For
FL-200815 Intragalactic communications using 6.3 PeV neutrinos
FL310715 Saraswati and the Neutron Stars - Stellar library and the flow of knowledge
FL-211212 Dyneraethitt Fermionik Rur Rineni - Advanced Fermionic Communications Protocols
FL-160415 Stellar Engineering: Technetium-based Beacons
Fox, D.B. The ANITA Anomalous Events as Signatures of a Beyond Standard Model Particle, and Supporting Observations from IceCube. arXiv:1809.09615v1. 2018.
Gorham, P.W. et al. [ANITA Collaboration], Phys. Rev. Lett. 117, no. 7, 071101 (2016).
Learned, J.G., Sandip Pakvasa, Zee, A. Galactic Neutrino Communication, (2008).
Pasachoff, J.M., Kutner, M.L. Neutrinos for Interstellar Communication. Cosmic Search 1, 2(1979).
Prasanta, K. ET AL. Neutrino Radar. 2002. http://arxiv.org/abs/hep-ph/0209057v1
Stancil, D.D. et al. Demonstration of communication using neutrinos. Modern Physics Letters A. World Scientific Publishing Company, 2012.
Subotowicz, M. Interstellar Communication by Neutrino Beams. Acta Astronautica 6, 213 (1979).>