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QUICK LOOK DATA

The most recent Voyager 6-hour averages for the LA1 (> 0.5 MeV/nuc nuclei) and PGH (> 70 MeV/nuc nuclei) rates are shown below in selectable thumbnail images.

The LA1 rate consists of greater than 0.5 MeV/nuc nuclei, principally protons, and is sensitive to low-energy phenomena in interplanetary space (e.g., co-rotating interaction regions, associated enhancements and solar flares).

The PGH rate consists of greater than 70 MeV/nuc nuclei, primarily protons, and is a good indicator of the level of modulation of galactic cosmic rays. It can also respond to large solar flares.

 

The Voyager 1 heater was turned off in May 2022. Corrections have been applied to the Voyager 1 flux data from DOY 145/2022 (May 25). Voyager 1 flux data from May 18 - 24 are not available.

The Voyager 2 heater was turned off in June 2019. Corrections have been applied to the Voyager 2 flux data from DOY 178/2019 (June 27). Voyager 2 flux data from DOY 160/2019 to DOY 178/2019 (June 9 - 26) are not available.

See Voyager Temperature Corrections for additional information.

The Rate data has not been corrected so please use caution using V1 Rate data after DOY 138/2022 (May 18) and V2 Rate data after DOY 159/2019 (June 8).

 

Voyager-1 3-Month >0.5 MeV/n Ions Rate Gif
Voyager-1 LA1 Rate
Voyager-1 3-Month >70 MeV/n Ions Rate Gif
Voyager-1 PGH Rate (HET 1)
Voyager-2 3-Month >0.5 MeV/n Ions Rate Gif
Voyager-2 LA1 Rate
Voyager-2 3-Month >70 MeV/n Ions Rate Gif
Voyager-2 PGH Rate (HET 1)

DATA INTERFACES

Through the Rate, Flux and Spectra User Interfaces you may generate figures and download CRS data for the lifetime of the Voyager mission. These interfaces have been tested with Microsoft Edge, Chrome and Firefox browsers.

 

Warning: Early misssion data (Voyager 1 and Voyager 2) contain Ground Communication Facility error flags. Data reprocessing in 2021 for the entire mission resulted in incorrect fluxes occasionally appearing in our public database when these flags are present. Data for 1984, 1985 and 1993 are particularly affected. The Voyager CRS team regenerated and uploaded correct data for 1992, 1993 and 1994. However, corrections for 1984 and 1985 are still in progress. Please use caution if you are working with data from 1984 and 1985.

DOCUMENTATION

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Last Updated: 11/18/2005