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{{Infobox spaceflight
{{Infobox spaceflight
| name = Solrad 8
| name = Solrad 8
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| Harvard_designation =
| Harvard_designation =
| SATCAT = 1738
| SATCAT = 1738
| mission_duration = Unknown
| mission_duration = {{time interval|November 19, 1965, 22:11:30}} (in orbit)
| COSPAR_ID = 1965-093A
| COSPAR_ID = 1965-093A
| spacecraft_bus =
| spacecraft_bus =
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| power =
| power =


| launch_date = {{start-date|November 19, 1965, 22:11:30|timezone=yes}}&nbsp;UTC <ref>{{cite web|url=http://rammb.cira.colostate.edu/dev/hillger/solar-observing.htm |title=Solar-observing satellites |publisher=Rammb.cira.colostate.edu |date= |accessdate=2014-05-27}}</ref>
| launch_date = {{start-date|November 19, 1965, 22:11:30|timezone=yes}}&nbsp;UTC <ref>{{cite web|url=http://rammb.cira.colostate.edu/dev/hillger/solar-observing.htm |title=Solar-observing satellites |publisher=Rammb.cira.colostate.edu |access-date=2014-05-27}}</ref><ref name="JSR">{{cite web|url=https://planet4589.org/space/log/launchlog.txt|title=Launch Log|publisher=Jonathan's Space Report |date=21 July 2021|access-date=9 November 2021}}</ref>
| launch_rocket = [[Scout (rocket)]]
| launch_rocket = [[Scout (rocket)|Scout X-4]]
| launch_site = [[Wallops Flight Facility Launch Area 3|Wallops LA-3]]
| launch_site = [[Wallops Flight Facility Launch Area 3|Wallops LA-3]]


| last_contact = {{end-date|August 1967}}
| last_contact = {{end-date|August 1967}}
| decay_date = Unknown
| decay_date =


| orbit_epoch = 19 November 1965, 04:48:00&nbsp;UTC
| orbit_epoch = 19 November 1965, 04:48:00&nbsp;UTC
| orbit_reference = [[geocentric orbit|Geocentric]]<ref name="Trajectory">{{cite web|url=https://nssdc.gsfc.nasa.gov/nmc/spacecraft/displayTrajectory.action?id=1965-093A|title=Trajectory: Explorer 30 (Solrad 8) 1965-093A|publisher=NASA|date=28 October 2021|access-date=9 November 2021}} {{PD-notice}}</ref>
| orbit_reference = [[geocentric orbit|Geocentric]]
| orbit_regime = [[Circular orbit]]
| orbit_regime = [[Circular orbit]]
| orbit_periapsis = {{convert|704|km|mi|sp=us}}
| orbit_periapsis = {{convert|704|km|mi|sp=us}}
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| orbit_rev_number =
| orbit_rev_number =
| apsis = gee
| apsis = gee

| programme = [[Explorers program|Explorers]]
| previous_mission = [[Explorer 29]]
| next_mission = [[Explorer 31]]
| programme2 = [[SOLRAD]]
| previous_mission2 = [[SOLRAD|Solrad 7B]]
| next_mission2 = [[Solrad 9]]
}}
}}
The '''SOLRAD 8''' satellite was one of the SOLRAD (Solar Radiation) program that began in 1960 to provide continuous coverage of solar radiation with a set of standard [[photometer]]s. SOLRAD 8 was a [[spin-stabilisation|spin-stabilized]] satellite oriented with its spin axis perpendicular to the sun-satellite line so that the 14 solar X-ray<ref>ftp://ftp.ngdc.noaa.gov/STP/SOLAR_DATA/SATELLITE_ENVIRONMENT/XRAY_BGND/docs/solrad.txt</ref> and ultraviolet photometers<ref>{{cite web|url=http://www.designation-systems.net/dusrm/app3/solrad.html |title=Solrad |publisher=Designation-systems.net |date= |accessdate=2014-05-27}}</ref> pointing radially outward from its equatorial belt viewed the sun on each revolution. Data were transmitted in real time by means of an FM/AM the satellite's telemetry system and were recorded by the stations on the [[STADAN]] tracking network.


The '''SOLRAD 8''','''Explorer 30''' or '''SE-A''' satellite was one of the [[NASA]] [[Solrad|SOLRAD]] (Solar Radiation) program that began in 1960 to provide continuous coverage of solar radiation with a set of standard [[photometer]]s. SOLRAD 8 was a [[spin-stabilisation|spin-stabilized]] satellite oriented with its [[spin axis]] perpendicular to the sun-satellite line so that the 14 solar X-ray<ref>ftp://ftp.ngdc.noaa.gov/STP/SOLAR_DATA/SATELLITE_ENVIRONMENT/XRAY_BGND/docs/solrad.txt</ref> and ultraviolet photometers<ref>{{cite web|url=http://www.designation-systems.net/dusrm/app3/solrad.html |title=Solrad |publisher=Designation-systems.net |access-date=2014-05-27}}</ref> pointing radially outward from its equatorial belt viewed the sun on each revolution. Data were transmitted in real time by means of an [[FM broadcasting|FM]] / [[Amplitude modulation|AM]] the satellite's telemetry system and were recorded by the stations on the [[Spacecraft Tracking and Data Acquisition Network]] (STADAN) tracking network.<ref name="Display">{{cite web |url=https://nssdc.gsfc.nasa.gov/nmc/spacecraft/display.action?id=1965-093A|title=Display: Explorer 30 (Solrad 8) 1965-093A|publisher=NASA|date=28 October 2021|access-date=9 November 2021}} {{PD-notice}}</ref>
The satellite observed the solar eclipse on May 20, 1966.<ref name="doi1">{{Cite journal | doi = 10.1038/211393a0| title = Solar Eclipse of May 20, 1966, observed by the Solrad 8 Satellite in X-ray and Ultra-violet Bands| journal = Nature| volume = 211| issue = 5047| pages = 393| year = 1966| last1 = Landini | first1 = M.| last2 = Russo | first2 = D.| last3 = Tagliaferri | first3 = G. L.}}</ref> This observation may have been the first observation of a [[solar eclipse]] by an [[artificial satellite]].<ref name="doi1" />


== Eclipse 1966 ==
The satellite performed nominally, except for the spin system,<ref>{{cite web|url=http://spacearchaeology.org/?p=436 |title=SOLRAD 8 |publisher=Space Archaeology |date= |accessdate=2014-05-27}}</ref> which failed to maintain 60 rpm (at spin rates below 10 rpm data reduction became difficult). The spin rate gradually decreased to 4 rpm on September 12, 1966.<ref>{{cite book|url=https://books.google.com/books?id=3WIrAAAAYAAJ&pg=PA47&lpg=PA47&dq=solrad+8&source=bl&ots=4MM0Jd9Hqx&sig=vcGWpaOplihAt_Qv6kCXDTcLklQ&hl=en&sa=X&ei=4_mEU7rkEc6LyASwjYKQBA&ved=0CG8Q6AEwCA#v=onepage&q=solrad%208&f=false|title=United States Space Science Program: Report to COSPAR.|publisher=National Academies|year=1967|author=National Research Council (U.S.). Space Science Board, COSPAR|page=47}}</ref> At that time, ground command succeeded in reactivating spinup to 78 rpm, which exhausted the gas supply. From this point, the spin rate gradually decreased to 10 rpm in August 1967, when data collection was substantially decreased.<ref>{{cite web|url=http://history.nasa.gov/SP-4312/ch1.htm |title=NASA:SP-4312 Dreams, Hopes, Realities-Chapter 1:Goddard's First Forty: The Quest to Learn |publisher=History.nasa.gov |date=1957-10-04 |accessdate=2014-05-27}}</ref>
The satellite observed the solar eclipse on 20 May 1966.<ref name="doi1">{{cite journal|doi=10.1038/211393a0|title=Solar Eclipse of 20 May 1966, observed by the Solrad 8 Satellite in X-ray and Ultraviolet Bands |journal=Nature|volume=211|issue=5047|page=393|year=1966|last1=Landini|first1=M.|last2=Russo|first2=D.|last3=Tagliaferri|first3=G. L.|bibcode=1966Natur.211..393L|s2cid=4174785}}</ref> This observation may have been the first observation of a [[solar eclipse]] by an [[artificial satellite]].<ref name="doi1"/>


==References==
== Mission ==

{{Include-NASA}}
The satellite performed normally, except for the spin system,<ref>{{cite web |url=http://spacearchaeology.org/?p=436 |title=SOLRAD 8 |publisher=Space Archaeology |access-date=2014-05-27 |archive-date=2017-12-08 |archive-url=https://web.archive.org/web/20171208003936/http://spacearchaeology.org/?p=436 |url-status=dead }}</ref> which failed to maintain 60 rpm (at spin rates below 10 rpm data reduction became difficult). The spin rate gradually decreased to 4 rpm on September 12, 1966.<ref>{{cite book|url=https://archive.org/details/bub_gb_3WIrAAAAYAAJ|title=United States Space Science Program: Report to COSPAR.|publisher=National Academies|year=1967|author=National Research Council (U.S.). Space Science Board, COSPAR|page=[https://archive.org/details/bub_gb_3WIrAAAAYAAJ/page/n53 47]}}</ref> At that time, ground command succeeded in reactivating spinup to 78 rpm, which exhausted the gas supply. From this point, the spin rate gradually decreased to 10 rpm in August 1967, when data collection was substantially decreased.<ref>{{cite web|url=https://history.nasa.gov/SP-4312/ch1.htm |title=NASA:SP-4312 Dreams, Hopes, Realities-Chapter 1:Goddard's First Forty: The Quest to Learn |publisher=History.nasa.gov |date=1957-10-04 |access-date=2014-05-27}}</ref>
{{reflist}}

== Experiment ==
=== Solar X-Ray and Ultraviolet Monitor ===
This experiment was designed to monitor solar X-ray and ultraviolet emissions with a set of standardized detectors so that the data could be compared directly with that produced by other experiments in the SOLRAD series. Eight [[Ionization chamber|ion chambers]] and two [[Geiger counter]]s covering the spectral regions from 0.5 [[Angstrom|A]] to 60 A and 1080 A to 1350 A were mounted perpendicular to the satellite spin axis. Analog outputs from the detectors were transmitted continuously on six IRIG telemetry channels. The experiment provided good data for all detectors from 27 November 1965 to 24 August 1967, with the following exceptions: (1) the Lyman-alpha detector and the UV detectors were saturated for normal aspect angles, (2) the core memory failed at launch so that the data were collected in real-time telemetry only, and (3) a gradual decrease in spin rate caused the aspect angle to drift away from normal in the second year of operation.<ref name="Experiment1">{{cite web |url=https://nssdc.gsfc.nasa.gov/nmc/experiment/display.action?id=1965-093A-01|title=Experiment: Solar X-Ray and Ultraviolet Monitor|publisher=NASA|date=28 October 2021|access-date=9 November 2021}} {{PD-notice}}</ref>


==See also==
==See also==
{{Portal|Spaceflight}}
*[[Explorers program]]
*[[Explorers program]]

==References==
{{Include-NASA}}
{{reflist}}


==External links==
==External links==
* http://www.techarchive.org/solrad-satellites/
* http://www.techarchive.org/solrad-satellites/
* [http://nssdc.gsfc.nasa.gov/nmc/datasetSearch.do?spacecraft=SOLRAD%20%208 NSSDC Solrad 8 data collections]
* [https://web.archive.org/web/20080920041827/http://nssdc.gsfc.nasa.gov/nmc/datasetSearch.do?spacecraft=SOLRAD%20%208 NSSDC Solrad 8 data collections]


{{Explorer program}}
{{Explorer program}}
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{{Use American English|date=January 2014}}
{{Use American English|date=January 2014}}


[[Category:Explorers program (NASA)]]
[[Category:Explorers Program]]
[[Category:Spacecraft launched in 1965]]
[[Category:Spacecraft launched in 1965]]
[[Category:Artificial satellites formerly orbiting Earth]]
[[Category:Satellites formerly orbiting Earth]]

Latest revision as of 04:50, 12 February 2024

Solrad 8
Mission typeSolar science
OperatorNASA
COSPAR ID1965-093A Edit this at Wikidata
SATCAT no.1738
Mission duration58 years, 8 months and 20 days (in orbit)
Spacecraft properties
ManufacturerNaval Research Lab
Launch mass56.7 kilograms (125 lb)
Start of mission
Launch dateNovember 19, 1965, 22:11:30 (1965-11-19UTC22:11:30Z) UTC [1][2]
RocketScout X-4
Launch siteWallops LA-3
End of mission
Last contactAugust 1967 (1967-09)
Orbital parameters
Reference systemGeocentric[3]
RegimeCircular orbit
Eccentricity0.01302
Perigee altitude704 kilometers (437 mi)
Apogee altitude891 kilometers (554 mi)
Inclination59.7 degrees
Period100.8 minutes
Epoch19 November 1965, 04:48:00 UTC

The SOLRAD 8,Explorer 30 or SE-A satellite was one of the NASA SOLRAD (Solar Radiation) program that began in 1960 to provide continuous coverage of solar radiation with a set of standard photometers. SOLRAD 8 was a spin-stabilized satellite oriented with its spin axis perpendicular to the sun-satellite line so that the 14 solar X-ray[4] and ultraviolet photometers[5] pointing radially outward from its equatorial belt viewed the sun on each revolution. Data were transmitted in real time by means of an FM / AM the satellite's telemetry system and were recorded by the stations on the Spacecraft Tracking and Data Acquisition Network (STADAN) tracking network.[6]

Eclipse 1966

[edit]

The satellite observed the solar eclipse on 20 May 1966.[7] This observation may have been the first observation of a solar eclipse by an artificial satellite.[7]

Mission

[edit]

The satellite performed normally, except for the spin system,[8] which failed to maintain 60 rpm (at spin rates below 10 rpm data reduction became difficult). The spin rate gradually decreased to 4 rpm on September 12, 1966.[9] At that time, ground command succeeded in reactivating spinup to 78 rpm, which exhausted the gas supply. From this point, the spin rate gradually decreased to 10 rpm in August 1967, when data collection was substantially decreased.[10]

Experiment

[edit]

Solar X-Ray and Ultraviolet Monitor

[edit]

This experiment was designed to monitor solar X-ray and ultraviolet emissions with a set of standardized detectors so that the data could be compared directly with that produced by other experiments in the SOLRAD series. Eight ion chambers and two Geiger counters covering the spectral regions from 0.5 A to 60 A and 1080 A to 1350 A were mounted perpendicular to the satellite spin axis. Analog outputs from the detectors were transmitted continuously on six IRIG telemetry channels. The experiment provided good data for all detectors from 27 November 1965 to 24 August 1967, with the following exceptions: (1) the Lyman-alpha detector and the UV detectors were saturated for normal aspect angles, (2) the core memory failed at launch so that the data were collected in real-time telemetry only, and (3) a gradual decrease in spin rate caused the aspect angle to drift away from normal in the second year of operation.[11]

See also

[edit]

References

[edit]

Public Domain This article incorporates public domain material from websites or documents of the National Aeronautics and Space Administration.

  1. ^ "Solar-observing satellites". Rammb.cira.colostate.edu. Retrieved 2014-05-27.
  2. ^ "Launch Log". Jonathan's Space Report. 21 July 2021. Retrieved 9 November 2021.
  3. ^ "Trajectory: Explorer 30 (Solrad 8) 1965-093A". NASA. 28 October 2021. Retrieved 9 November 2021. Public Domain This article incorporates text from this source, which is in the public domain.
  4. ^ ftp://ftp.ngdc.noaa.gov/STP/SOLAR_DATA/SATELLITE_ENVIRONMENT/XRAY_BGND/docs/solrad.txt
  5. ^ "Solrad". Designation-systems.net. Retrieved 2014-05-27.
  6. ^ "Display: Explorer 30 (Solrad 8) 1965-093A". NASA. 28 October 2021. Retrieved 9 November 2021. Public Domain This article incorporates text from this source, which is in the public domain.
  7. ^ a b Landini, M.; Russo, D.; Tagliaferri, G. L. (1966). "Solar Eclipse of 20 May 1966, observed by the Solrad 8 Satellite in X-ray and Ultraviolet Bands". Nature. 211 (5047): 393. Bibcode:1966Natur.211..393L. doi:10.1038/211393a0. S2CID 4174785.
  8. ^ "SOLRAD 8". Space Archaeology. Archived from the original on 2017-12-08. Retrieved 2014-05-27.
  9. ^ National Research Council (U.S.). Space Science Board, COSPAR (1967). United States Space Science Program: Report to COSPAR. National Academies. p. 47.
  10. ^ "NASA:SP-4312 Dreams, Hopes, Realities-Chapter 1:Goddard's First Forty: The Quest to Learn". History.nasa.gov. 1957-10-04. Retrieved 2014-05-27.
  11. ^ "Experiment: Solar X-Ray and Ultraviolet Monitor". NASA. 28 October 2021. Retrieved 9 November 2021. Public Domain This article incorporates text from this source, which is in the public domain.
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