"WMAP News: Facts". NASA. 22 April 2008. สืบค้นเมื่อ 27 April 2008.
"Wilkinson Microwave Anisotropy Probe: Overview". Legacy Archive for Background Data Analysis (LAMBDA). Greenbelt, Maryland: NASA's High Energy Astrophysics Science Archive Research Center (HEASARC). August 4, 2009. สืบค้นเมื่อ 24 September 2009. The WMAP (Wilkinson Microwave Anisotropy Probe) mission is designed to determine the geometry, content, and evolution of the universe via a 13 arcminute FWHM resolution full sky map of the temperature anisotropy of the cosmic microwave background radiation.
"Tests of Big Bang: The CMB". Universe 101: Our Universe. NASA. July 2009. สืบค้นเมื่อ 24 September 2009. Only with very sensitive instruments, such as COBE and WMAP, can cosmologists detect fluctuations in the cosmic microwave background temperature. By studying these fluctuations, cosmologists can learn about the origin of galaxies and large scale structures of galaxies and they can measure the basic parameters of the Big Bang theory.
↑ "New image of infant universe reveals era of first stars, age of cosmos, and more". NASA / WMAP team. 11 February 2003. สืบค้นเมื่อ 27 April 2008.
ดาวเท, ยมสำรวจคล, นไมโครเวฟว, ลก, นส, งกฤษ, wilkinson, microwave, anisotropy, probe, wmap, หร, ดาวเท, ยมด, บเบ, ลย, แมป, อเด, มค, แมป, และ, เอ, กพลอเรอร, explorer, เป, นยานอวกาศท, ดความแตกต, างของอ, ณหภ, การแผ, งส, ความร, อนท, หลงเหล, ออย, จากเหต, การณ, กแบง, . dawethiymsarwckhlunimokhrewfwilkinsn xngkvs Wilkinson Microwave Anisotropy Probe WMAP hrux dawethiymdbebilyuaemp chuxedimkhux aemp MAP aela exkphlxerxr 80 Explorer 80 epnyanxwkasthiwdkhwamaetktangkhxngxunhphumikaraephrngsikhwamrxnthihlngehluxxyucakehtukarnbikaebng hruxthieriykwa karaephrngsiimokhrewfphunhlngkhxngckrwal odykartrwcwdipthwthxngfa 4 5 hwhnaokhrngkarkhuxsastracary charls aexl ebnentt aehngmhawithyalycxhnhxpkins odyepnokhrngkarkhwamrwmmuxrahwangsunykarbinxwkaskxdedird xngkhkarnasa kbmhawithyalyphrinstn 6 yanxwkasdbebilyuaempthuknasngkhunxwkasemux 30 mithunayn kh s 2001 cakflxrida ptibtikardbebilyuaempprasbkhwamsaercinpharkic COBE aelacdepnyanxwkasradbklang MIDEX lathisxngkhxngokhrngkarsarwcxwkas inpi kh s 2003 chuxokhrngkarepliyncak MAP maepn WMAP ephuxepnkarihekiyrtiaek edwid thxdd wilkinsn kh s 1935 2002 6 smachikkhnhnunginkhnankwithyasastrinokhrngkarnidawethiymsarwckhlunimokhrewfwilkinsnkhxmulthwipchuxxun MAP Explorer 80rhs NSSDC 2001 027AxngkhkrNASAwnkhunsuxwkas 30 mithunayn 2001 19 46 UTCkhuncak thanthphxakasaehlmkhanaewxrlyankhnsng Delta II 7425 10rayaewlapharkic phanmaaelw 20 pi 1 eduxn 5 wnmwl840 kgpraephthwngokhcr Lissajous orbittaaehnngaemaebb L2ekhruxngmux K band 23 GHz 52 8 MOA beamKa band 33 GHz 39 6 MOA beamQ band 41 GHz 30 6 MOA beamV band 61 GHz 21 MOA beamW band 94 GHz 13 2 MOA beam ewbisthttp map gsfc nasa govReferences 1 2 3 xangxing aekikh Bennett C 2003 The Microwave Anisotropy Probe MAP Mission Astrophysical Journal 583 1 23 doi 10 1086 345346 Unknown parameter coauthors ignored author suggested help Limon M 20 March 2008 Wilkinson Microwave Anisotropy Probe WMAP Five Year Explanatory Supplement PDF Unknown parameter coauthors ignored author suggested help WMAP News Facts NASA 22 April 2008 subkhnemux 27 April 2008 Wilkinson Microwave Anisotropy Probe Overview Legacy Archive for Background Data Analysis LAMBDA Greenbelt Maryland NASA s High Energy Astrophysics Science Archive Research Center HEASARC August 4 2009 subkhnemux 24 September 2009 The WMAP Wilkinson Microwave Anisotropy Probe mission is designed to determine the geometry content and evolution of the universe via a 13 arcminute FWHM resolution full sky map of the temperature anisotropy of the cosmic microwave background radiation Tests of Big Bang The CMB Universe 101 Our Universe NASA July 2009 subkhnemux 24 September 2009 Only with very sensitive instruments such as COBE and WMAP can cosmologists detect fluctuations in the cosmic microwave background temperature By studying these fluctuations cosmologists can learn about the origin of galaxies and large scale structures of galaxies and they can measure the basic parameters of the Big Bang theory 6 0 6 1 New image of infant universe reveals era of first stars age of cosmos and more NASA WMAP team 11 February 2003 subkhnemux 27 April 2008 aehlngkhxmulxun aekikhkhxmmxns miphaphaelasuxekiywkb dawethiymsarwckhlunimokhrewfwilkinsnSizing up the universe ekiywkb WMAP aelarngsiimokhrewfphunhlngkhxngckrwal bthkhwamthi Space com Big Bang glow hints at funnel shaped Universe NewScientist 15 emsayn 2004 NASA 16 minakhm 2006 khawprachasmphnthekiywkbkarlxytwkhxng WMAP Seife Charles 2003 With Its Ingredients MAPped Universe s Recipe Beckons Science 300 5620 730 731 doi 10 1126 science 300 5620 730 PMID 12730575 bthkhwamekiywkbdarasastrhruxckrwalwithyaniyngepnokhrng khunsamarthchwywikiphiediyidodyephimkhxmul duephimthi sthaniyxy darasastrekhathungcak https th wikipedia org w index php title dawethiymsarwckhlunimokhrewfwilkinsn amp oldid 8995528, wikipedia, วิกิ หนังสือ, หนังสือ, ห้องสมุด,
