2025 ISR World Days

This page lists the 2025 Incoherent Scatter Radar (ISR) World Days. ISR World Days are days in which multiple ISRs simultaneously take observations for science needs that are global in nature. To create this schedule, proposals are first solicited yearly within the space physics. These proposals are then discusses amongest the public, ISR PIs, and the URSI Incoherent Scatter Working Group at a 'town hall'. Then, approved proposals are scheduled for the following year. Please reach out if you have any questions!
Month New Moon Full Moon Experiment Experiment Length
December 2024 1, 30 15

Dynamics

10 Days
January 29 13

Dynamics

10 Days
February 27 12
1 to 14

Dynamics

10 Days
19 to 28

ICME

5 Days
March 29 14
1 to 7

ICME

5 Days
8 to 17

Dynamo

5 Days
17 to 31

ICME

5 Days
April 27 12

Dynamo

5 Days
May 26 12

Dynamo

5 Days
June 25 11
July 24 10
August 23 9
September 21 7

CONGS-25

5 Days
October 21 6

CONGS-25

5 Days
November 20 5
December 19 4

Dynamics: Dynamics, electrodynamics, temperature and electron density in the lower and upper thermosphere and ionosphere during strong polar vortex conditions

Requester: Goncharenko
Primary Parameters to Measure, including requested time resolution: Electron density, electron and ion temperatures from lowest possible altitude throughout the F-region. Temporal resolution can be sacrificed and data integration period increased in order to obtain data at lower altitudes.
Secondary Parameters to Measure: Zonal and meridional components of neutral wind in the lower thermosphere (95-140km), ExB drift, F-region meridional wind.
Requested radars: PFISR, RISR-N, RISR-C, EISCAT (mainland and Svalbard), Millstone Hill, Jicamarca, Kharkiv, QJISR, and PANSY.
NOTE 1: A 10-day campaign on alert basis is requested, with alert window Dec 15 – Feb 15. The decision to start will be based on predictions of stratospheric conditions. In the case of no anomalous stratospheric conditions (strong polar vortex or sudden stratospheric warming event), the World Day will revert to a 5‐day run at the end of the alert period, 9‐14 February. There should be one week's notice for the alert

ICME: Geomagnetic storm triggered by ICME

Requester: Aikio
Primary Parameters to Measure, including requested time resolution: Plasma parameters: Ne, Te, Ti, Vi, (the basic time resolution of the measurement) 1 min or shorter.
Secondary Parameters to Measure: Ion velocity vectors and electric fields (analyzed from ion velocity measurements along several directions in the F-region), time resolution 1-5 min.
Requested radars: PFISR, RISR-N, RISR-C, EISCAT (mainland and Svalbard), Millstone Hill
NOTE 2: On alert after CME, alert periods avoiding full moon: 19 February -7 March 2025, 17 March – 31 March 2025, 5-day continuous (24-h) measurement

Dynamo: Solar wind-magnetosphere-ionosphere and thermosphere disturbance wind dynamo effects over the storm-time upper atmosphere dynamics and electrodynamics

Requester: Navarro
Primary Parameters to Measure, including requested time resolution: Plasma drifts throughout the F-region up to highest altitude possible. Temporal resolution of 5 mins depending on SNR. We might request reprocessing of data for 1-min resolution for specific time periods (mostly during daytime).
Secondary Parameters to Measure: Zonal and meridional thermospheric neutral winds from SDI and FPI support instrumentation at ISR locations or nearby. If possible, coherent backscatter observations from AMISR-14 system at Jicamarca for support of tracking irregularities at equatorial latitudes.
Requested radars: PFISR, RISR-N, RISR-C, EISCAT (mainland and Svalbard), Millstone Hill, Jicamarca, SYISR, QJISR, Kharkiv, Irkutsk, and PAANSY
A 5-days campaign on alert basis is requested, with alert window Mar 1 – May 30.

CONGS-25: 2025 Coordinated Observation of Geospace Storm (CONGS-25)

Requester: Zhang
Primary Parameters to Measure, including requested time resolution: Basic ISR parameters (Ne, Te, Ti, and Vo) with typical 2-3 min integration time. If possible, high temporal resolution plasma-line electron density data.
Secondary Parameters to Measure: Resolved ion velocity vector locally or regionally; thermospheric winds and temperature
Requested radars: PFISR, RISR-N, RISR-C, EISCAT (mainland and Svalbard), Millstone Hill, Jicamarca, Sanya, Kharkiv, QJISR, Irkutsk, and PANSY
A 5-day campaign on alert basis. The exact dates will be determined based on the geomagnetic activity forecasts. The PIs will communicate with the facilities, issue observation alerts and announce the kickoff time approximately 3 days ahead of the campaign start.