a prototype service to monitor the ionospheric scintillations

1
A prototype service to monitor the ionospheric scintillations J.J. Valette, P. Yaya, B. Nhun Fat (CLS) & P. Lassudrie-Duchesne, R. Fleury (ENSTB) ESA Pilot Project for Space Weather Applications PROCESSING PROCESSING PARTNERSHIP PARTNERSHIP SERVICE PROTOTYPE SERVICE PROTOTYPE CALIBRATION CALIBRATION KOUROU – seasonal/diurnal KOUROU – seasonal/diurnal variations variations YELLOWKNIFE: RINEX amplitude data (IGS, 1s samples) ——— S1 ——— S2 Ionospheric effect multipaths 2 2 4 / S P P P (P = 1 min average) 7 Nov. 2004 - 7 Nov. 2004 - Magnetic storm Magnetic storm monitoring monitoring Hourly maps Hourly maps - 1 s GPS data - 1 s GPS data (60 sites) (60 sites) Max activity expected during Max activity expected during the equinox the equinox 1-30 March 2004 (Kp max=6) 1-30 March 2004 (Kp max=6) Min activity expected during Min activity expected during the solstices the solstices 1-30 June 2004 (Kp max=5) 1-30 June 2004 (Kp max=5) GPS Permanent network perturbations analyses that lead to empirical GPS Permanent network perturbations analyses that lead to empirical scintillation index : scintillation index : - L2 signal tracking losses & cycle slips - L2 signal tracking losses & cycle slips - Phase fluctuations - Phase fluctuations - Signal-to-noise - Signal-to-noise 0 200 400 600 800 1000 1200 1400 m edium (0.25-0.5) strong (0.5-0.75) severe (>0.75) ASHTECH UZ-12 JPS LEG ACY 0 100 200 300 1 3 5 7 9 11 13 15 17 19 21 23 25 LocalTim e 0 100 200 300 1 3 5 7 9 11 13 15 17 19 21 23 25 LocalTim e 0 100 200 300 0 2 4 6 8 10 12 14 16 18 20 22 LocalTim e 0 100 200 300 1 3 5 7 9 11 13 15 17 19 21 23 LocalTim e 0 200 400 600 800 1000 1200 1400 m edium (0.25-0.5) strong (0.5-0.75) severe (>0.75) 2 permanent receivers (ESA/ESOC) at 2 permanent receivers (ESA/ESOC) at KOUROU: KOUROU: ASHTECH UZ-12 (kour) ASHTECH UZ-12 (kour) JPS LEGACY (kou1) JPS LEGACY (kou1) Scintillation intensity distribution Scintillation intensity distribution March 2004: about 3000 events (>0.25) March 2004: about 3000 events (>0.25) June 2004: about 100 events (>0.25) June 2004: about 100 events (>0.25) ASHTECH UZ-12 ASHTECH UZ-12 (kour, 30 s (kour, 30 s samples) samples) JPS LEGACY JPS LEGACY kou1, 30 s samples) kou1, 30 s samples) March 2004 March 2004 June 2004 June 2004 S1 and S2 amplitudes or phases RINEX data available from the IGS S1 and S2 amplitudes or phases RINEX data available from the IGS network need to be calibrated. The proposed calibration scheme network need to be calibrated. The proposed calibration scheme involves the use of a Ionospheric Scintillation Monitor (ISM) involves the use of a Ionospheric Scintillation Monitor (ISM) collocated with an IGS station. Some comparisons have been done collocated with an IGS station. Some comparisons have been done with an ESA ISM at Douala (Cameroon). Kourou will soon be with an ESA ISM at Douala (Cameroon). Kourou will soon be equiped with an ISM for this purpose. equiped with an ISM for this purpose. ROB Disturbances in the ionosphere especially in the equatorial Disturbances in the ionosphere especially in the equatorial region are due to strong irregularities on electron region are due to strong irregularities on electron concentration in the E and F regions. Typical turbulences concentration in the E and F regions. Typical turbulences associated with the scintillations of signals propagating in associated with the scintillations of signals propagating in the plasma medium have an extension of a few hundred the plasma medium have an extension of a few hundred meters and a characteristic period of the ions recombination meters and a characteristic period of the ions recombination processes from below 0.01s up to a few seconds. The processes from below 0.01s up to a few seconds. The phenomena may last several hours with major intensity phenomena may last several hours with major intensity after sunset (along the Equator). It produces strong and after sunset (along the Equator). It produces strong and rapid amplitude and phase fluctuations of a GPS rapid amplitude and phase fluctuations of a GPS propagating signal. propagating signal. 00h 00h TU TU Kp= 1 Kp= 1 21h 21h TU TU Kp= 6 Kp= 6 Kp= 2 Kp= 2 Kp= 9 Kp= 9 5 & 8 Nov. 2004 - 5 & 8 Nov. 2004 - Magnetic storm Magnetic storm monitoring monitoring Daily maps Daily maps - 30 s GPS data (250 - 30 s GPS data (250 sites) sites) First European Space Weather Week, First European Space Weather Week, Noordwijk, 29th Nov. - 3 Dec. Noordwijk, 29th Nov. - 3 Dec. 2004 2004 PRODUCTS PRODUCTS http://scintillations.cls.fr/ http://scintillations.cls.fr/

Upload: yardley

Post on 15-Jan-2016

35 views

Category:

Documents


1 download

DESCRIPTION

ROB. A prototype service to monitor the ionospheric scintillations J.J. Valette, P. Yaya, B. Nhun Fat (CLS) & P. Lassudrie-Duchesne, R. Fleury (ENSTB) ESA Pilot Project for Space Weather Applications. PARTNERSHIP. - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: A prototype service to monitor the ionospheric scintillations

A prototype service to monitor the ionospheric scintillations J.J. Valette, P. Yaya, B. Nhun Fat (CLS) & P. Lassudrie-Duchesne, R. Fleury (ENSTB)

ESA Pilot Project for Space Weather Applications

PROCESSINGPROCESSINGPROCESSINGPROCESSING

PARTNERSHIPPARTNERSHIPPARTNERSHIPPARTNERSHIP

SERVICE PROTOTYPESERVICE PROTOTYPESERVICE PROTOTYPESERVICE PROTOTYPE

CALIBRATIONCALIBRATIONCALIBRATIONCALIBRATION

KOUROU – seasonal/diurnal variationsKOUROU – seasonal/diurnal variationsKOUROU – seasonal/diurnal variationsKOUROU – seasonal/diurnal variations

• YELLOWKNIFE: RINEX amplitude data (IGS, 1s samples)

——— S1 ——— S2

Ionosphericeffect

multipaths

2 24 /S P P P

(P = 1 min average)

7 Nov. 2004 - 7 Nov. 2004 - Magnetic storm monitoringMagnetic storm monitoring

Hourly mapsHourly maps - 1 s GPS data (60 sites) - 1 s GPS data (60 sites)

Max activity expected during the equinoxMax activity expected during the equinox1-30 March 2004 (Kp max=6)1-30 March 2004 (Kp max=6)

Min activity expected during the solsticesMin activity expected during the solstices1-30 June 2004 (Kp max=5)1-30 June 2004 (Kp max=5)

GPS Permanent network perturbations analyses that lead to empirical scintillation index :GPS Permanent network perturbations analyses that lead to empirical scintillation index :- L2 signal tracking losses & cycle slips- L2 signal tracking losses & cycle slips- Phase fluctuations- Phase fluctuations- Signal-to-noise- Signal-to-noise

0

200

400

600

800

1000

1200

1400

medium (0.25-0.5) strong (0.5-0.75) severe (>0.75)

ASHTECH UZ-12

JPS LEGACY

0

100

200

300

1 3 5 7 9 11 13 15 17 19 21 23 25

Local Time

0

100

200

300

1 3 5 7 9 11 13 15 17 19 21 23 25

Local Time

0

100

200

300

0 2 4 6 8 10 12 14 16 18 20 22

Local Time

0

100

200

300

1 3 5 7 9 11 13 15 17 19 21 23

Local Time

0

200

400

600

800

1000

1200

1400

medium (0.25-0.5) strong (0.5-0.75) severe (>0.75)

2 permanent receivers (ESA/ESOC) at KOUROU:2 permanent receivers (ESA/ESOC) at KOUROU:ASHTECH UZ-12 (kour)ASHTECH UZ-12 (kour)JPS LEGACY (kou1)JPS LEGACY (kou1)

Scintillation intensity distributionScintillation intensity distributionMarch 2004: about 3000 events (>0.25)March 2004: about 3000 events (>0.25)

June 2004: about 100 events (>0.25)June 2004: about 100 events (>0.25)

ASHTECH UZ-12 ASHTECH UZ-12 (kour, 30 s samples)(kour, 30 s samples)

JPS LEGACY JPS LEGACY kou1, 30 s samples)kou1, 30 s samples)

March 2004March 2004

June 2004June 2004

S1 and S2 amplitudes or phases RINEX data available from the IGS network S1 and S2 amplitudes or phases RINEX data available from the IGS network need to be calibrated. The proposed calibration scheme involves the use of a need to be calibrated. The proposed calibration scheme involves the use of a Ionospheric Scintillation Monitor (ISM) collocated with an IGS station. Ionospheric Scintillation Monitor (ISM) collocated with an IGS station. Some comparisons have been done with an ESA ISM at Douala (Cameroon). Some comparisons have been done with an ESA ISM at Douala (Cameroon). Kourou will soon be equiped with an ISM for this purpose.Kourou will soon be equiped with an ISM for this purpose.

ROB

Disturbances in the ionosphere especially in the equatorial region are Disturbances in the ionosphere especially in the equatorial region are due to strong irregularities on electron concentration in the E and F due to strong irregularities on electron concentration in the E and F regions. Typical turbulences associated with the scintillations of regions. Typical turbulences associated with the scintillations of signals propagating in the plasma medium have an extension of a few signals propagating in the plasma medium have an extension of a few hundred meters and a characteristic period of the ions recombination hundred meters and a characteristic period of the ions recombination processes from below 0.01s up to a few seconds. The phenomena may processes from below 0.01s up to a few seconds. The phenomena may last several hours with major intensity after sunset (along the last several hours with major intensity after sunset (along the Equator). It produces strong and rapid amplitude and phase Equator). It produces strong and rapid amplitude and phase fluctuations of a GPS propagating signal.fluctuations of a GPS propagating signal.

00h TU00h TUKp= 1Kp= 1

21h TU21h TUKp= 6Kp= 6

Kp= 2Kp= 2

Kp= 9Kp= 9

5 & 8 Nov. 2004 - 5 & 8 Nov. 2004 - Magnetic storm monitoringMagnetic storm monitoring

Daily mapsDaily maps - 30 s GPS data (250 sites) - 30 s GPS data (250 sites)

First European Space Weather Week,First European Space Weather Week, Noordwijk, 29th Nov. - 3 Dec. 2004 Noordwijk, 29th Nov. - 3 Dec. 2004

PRODUCTSPRODUCTSPRODUCTSPRODUCTS

http://scintillations.cls.fr/http://scintillations.cls.fr/