Aditya L1 Update: PAPA Payload is Now Operational, PAPA Payload Data

Aditya L1 Update: PAPA Payload

PAPA payload ( Plasma Analyser Package for Aditya ) on Aditya L1 is now functioning at its maximum capacity of 5 Kv and has initiated the transmission of data of high quality. On 8 December 2023, the payload was switched on for the first time only for 10 hours during the cruise phase.

During the cruise phase, the functionality of the payload was assessed to evaluate its in-orbit condition. Both the primary and backup DC-DC converters were utilized for testing. It is noteworthy that the high voltage (5 kV) was not enabled during this specific cruise phase.

On December 11, 2023, ISRO planned to switch on the high voltage (5 kV) for the first time. The process was conducted gradually, step by step, with close monitoring of all parameters to ensure careful oversight. Now PAPA payload is healthy and sending good-quality data.

More About PAPA Payload

PAPA payload ( Plasma Analyser Package for Aditya )
PAPA payload ( Plasma Analyser Package for Aditya ) Credit: ISRO

The Plasma Analyser Package for Aditya (PAPA) installed on the Aditya-L1 spacecraft serves as an energy and mass analyzer payload designed to observe the flux of solar wind electrons and ions. It incorporates two sensors, namely the Solar Wind Electron Energy Probe (SWEEP) and the Solar Wind Ion Composition Analyser (SWICAR). Investigating the flux and energies of electrons and ions contributes to advancing our comprehension of solar dynamics, space weather events, and their potential effects on spacecraft and the solar system.

PAPA Payload Data

The payload has been in operation since December 12, 2023. Figure 1 displays its observations during the Halo Orbit Insertion (HOI) phase. The figure displays the time series of SWEEP electron energy spectra and total count observed throughout the Halo Orbit Insertion (HOI) phase, as well as the periods before and after it.

PAPA Payload Data
Figure1: The time series of SWEEP electron energy spectra spans from 04:00:30 UTC to 17:59:58 UTC on January 6, 2024, Including the Pre-HOI, HOI, and Post-HOI phases. The noticeable dip in the spectra is linked to the spacecraft’s rotation in the HOI phase, particularly when the sensor’s orientation is away from the Sun. Source: ISRO

Figure 2 presents the time series of SWICAR ion energy spectra and integrated counts within the designated timeframe. It showcases the anticipated patterns of ion energy spectra under typical space weather conditions.

PAPA Payload Data
The time series of SWICAR ion energy spectra and integrated counts, depicted in the top two panels, spans from 04:01:36 UTC to 17:58:53 UTC on January 6, 2024. The presentation illustrates variations across the Pre-HOI, HOI, and Post-HOI phases. Source: ISRO

The PAPA payload data indicated the presence of Coronal Mass Ejection (CME) incidents, notably on December 15, 2023, and between February 10 and 11, 2024, as depicted in Figures 3 and 4. The CME occurrence on December 15, 2023, was singular. Conversely, the fluctuations observed in electron and ion counts during February 10-11, 2024, stem from several minor events, each showcasing distinct time variations in electron and ion counts.

PAPA Payload Data
Figure 3: The time series displays the integrated raw counts for (a) solar wind electrons, recorded by the PAPA-SWEEP sensor, and (b) solar wind ions, measured by the PAPA-SWICAR sensor, spanning from 05:45:00 UT on December 15 to 23:55:00 UT on December 16, 2023. Source: ISRO
PAPA Payload Data
Figure 2: Similar to Figure 3, this figure represent the CMEs that occurred between February 10 and 11, 2024.
Source: ISRO

For more details visit ISRO source.

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