Pioneers 6, 7, 8, and 9 were created to make the first detailed, comprehensive measurements of the solar wind, solar magnetic field and cosmic rays. They were designed to measure large scale magnetic phenomena and particles and fields in interplanetary space. Data from the vehicles have been used to better understand stellar processes and the structure and flow of the solar wind. The vehicles also acted as the world's first space-based solar weather network, providing practical data on solar storms which affect communications and power on Earth.2
The experiments studied the positive ions (cations) and electrons in the solar wind, the interplanetary electron density (radio propagation experiment), solar and galactic cosmic rays, and the Interplanetary Magnetic Field.3
The spacecraft were important collectors of heliophysics and space weather data. In conjunction with other spacecraft these, for the first time, enabled spaceborne observations to be combined with terrestrial observations on the ground and from sounding balloons. In early August 1972 Pioneer 9 recorded significant observations of one of the most potent solar storms ever recorded, and the most hazardous to human spaceflight during the Space Age.4
Each craft was identical. They were spin-stabilized 0.94 m (3 ft 1 in) diameter × 0.81 m (2 ft 8 in) tall cylinders with a 1.8 m (5 ft 11 in) long magnetometer boom and solar panels mounted around the body.
The main antenna was a high-gain directional antenna. The spacecraft were spin-stabilized at about 60 RPM, and the spin axis was perpendicular to the ecliptic plane and pointed toward the south ecliptic pole.5
Instruments differed somewhat between spacecraft, with some being used in all four missions:
By ground command, one of five bit rates, one of four data formats, and one of four operating modes could be selected. The five-bit rates were 512, 256, 64, 16, and 8 bit/s. Three of the four data formats contained primarily scientific data and consisted of 32 seven-bit words per frame. One scientific data format was for use at the two highest bit rates. Another was for use at the three lowest bit rates. The third contained data from only the radio propagation experiment. The fourth data format contained mainly engineering data.6
The four operating modes were: real-time, telemetry store, duty cycle store, and memory readout. In the real-time mode, data were sampled and transmitted directly (without storage) as specified by the data format and bit rate selected. In the telemetry store mode, data were stored and transmitted simultaneously in the format and at the bit rate selected. In the duty-cycle store mode, a single frame of scientific data was collected and stored at a rate of 512 bit/s. The time interval between the collection and storage of successive frames could be varied by ground command between 2 and 17 min to provide partial data coverage for periods up to 19 hours, as limited by the bit storage capacity. In the memory readout mode, data was read out at whatever bit rate was appropriate to the satellite distance from Earth.7
As stated by JPL, "The Pioneer 6–9 program has been touted as one of the least expensive of all NASA spacecraft programs in terms of scientific results per dollar spent."8 Although the four spacecraft have not been regularly tracked for science data return in recent years, a successful telemetry contact with Pioneer 6 was made on December 8, 2000, to celebrate 35 years of continuous operation since launch. Its original design life expectancy was only 6 months.
Although NASA described Pioneer 6 as "extant" as of 26 March 2007,9 there has been no contact since December 8, 2000. At this time Pioneer 6 had operated for 12,758 days, making it the oldest operating space probe until it was surpassed by Voyager 2 on August 13, 2012.10 It is also believed that contact is still possible with Pioneer 7 and 8; only Pioneer 9 is definitely not working.
"Pioneer 6". nssdc.gsfc.nasa.gov. NASA. Archived from the original on August 4, 2021. Retrieved September 9, 2018. This article incorporates text from this source, which is in the public domain. https://nssdc.gsfc.nasa.gov/nmc/spacecraft/display.action?id=1965-105A ↩
D. J. Knipp; B. J. Fraser; M. A. Shea; D. F. Smart (2018). "On the Little‐Known Consequences of the 4 August 1972 Ultra-Fast Coronal Mass Ejecta: Facts, Commentary and Call to Action". Space Weather. 16 (11): 1635–1643. Bibcode:2018SpWea..16.1635K. doi:10.1029/2018SW002024. https://doi.org/10.1029%2F2018SW002024 ↩
"Pioneer 6, 7, 8, 9, E - Quicklook". Jet Propulsion Laboratory. Archived from the original on July 21, 2010. https://web.archive.org/web/20100721112116/http://msl.jpl.nasa.gov/QuickLooks/pioneer6QL.html ↩
"The Pioneer Missions". nasa.gov. NASA. Archived from the original on August 15, 2011. Retrieved August 27, 2009. https://web.archive.org/web/20110815233221/http://www.nasa.gov/centers/ames/missions/archive/pioneer.html ↩
"Voyager at 35 - Break on Through to the Other Side". nasa.gov. NASA. Archived from the original on March 8, 2015. Retrieved May 5, 2015. https://www.nasa.gov/mission_pages/voyager/voyager20120820.html ↩
J. D. Mihalov; H. R. Collard; D. S. Intriligator; A. Barnes (1987). "Observation by Pioneer 7 of He+ in the distant coma of Halley's Comet". Icarus. 71 (1): 192–197. Bibcode:1987Icar...71..192M. doi:10.1016/0019-1035(87)90172-2. /wiki/Bibcode_(identifier) ↩
"Pioneer 8". nssdc.gsfc.nasa.gov. NASA. Archived from the original on June 29, 2019. Retrieved February 27, 2022. https://nssdc.gsfc.nasa.gov/nmc/spacecraft/display.action?id=1967-123A ↩
"Pioneer 9 - NASA Science". science.nasa.gov. NASA. Retrieved March 6, 2019. https://science.nasa.gov/mission/pioneer-9/ ↩