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ARL Applied Research Laboratories The University of Texas at Austin ARL Applied Research Laboratories The University of Texas at Austin Ionospheric Tomography.

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Presentation on theme: "ARL Applied Research Laboratories The University of Texas at Austin ARL Applied Research Laboratories The University of Texas at Austin Ionospheric Tomography."— Presentation transcript:

1 ARL Applied Research Laboratories The University of Texas at Austin ARL Applied Research Laboratories The University of Texas at Austin Ionospheric Tomography Network of Egypt T W Garner Applied Research Laboratories University of Texas at Austin A M Mahrous Space Weather Monitoring Center Helwan University

2 ARL Applied Research Laboratories The University of Texas at Austin Ionospheric Tomography Network of Egypt Chain of 3 CIDRs in Egypt as part of ISWI Only 1 is operational right now Located at different university campuses across Egypt. Operated jointly by Helwan University (Ayman Mahrous) and ARL:UT (Trevor Garner)

3 ARL Applied Research Laboratories The University of Texas at Austin UHF/VHF Satellite Radio Beacons  Transit-  First satellite navigation system  Satellites in LEO (~1000 km), polar orbit  Transmitted navigation message at 150 and 400 MHz  Doppler shift of the signals used for positioning  Decommissioned in 1989 to the Navy Ionospheric Monitoring System (NIMS)  4 Active beacons  Other US Radio Beacons-  Several DoD missions have flown a NRL-developed radio beacon  C/NOFS, DMSP F15, Radcal  Several other nations have flown or will fly radio beacons  COSMIC, ePoP, future Brazilian and Indian missions

4 Coherent Ionospheric Doppler Receivers (CIDRs)  Designed to track 150/400MHz LEO beacons (Transit/NIMS, GFO)  Provides relative TEC and phase scintillation measurements  Useful for examining spatial structure with a relatively sparse receiver network and conducting ionospheric tomography 30 meter RF cable 150 MHz 400 MHz PCRX

5 ARL Applied Research Laboratories The University of Texas at Austin CIDR measurements  Doppler shift in both the 150 and 400 MHz channels  Linear combinations of these two Doppler shifts produce three separate ionospheric measurements  STEC/  t  Ionospheric δf at 150 MHz  Ionospheric δf at 400 MHz  The  STEC/  t can be integrated to a STEC under the satellite  All three measurements can be binned and RMS values used to characterize the scintillation

6 ARL Applied Research Laboratories The University of Texas at Austin Ionospheric Doppler Shift

7 ARL Applied Research Laboratories The University of Texas at Austin Dual Frequency Combinations  Most existing UHF/VHF beacons transmit at 8/3  There are 2 basic linear combinations for dual frequency Doppler measurements

8 ARL Applied Research Laboratories The University of Texas at Austin Scale of CIDR measurements  For a typical beacon satellite orbit, the satellite crosses a full field of view in 20 minutes.  Corresponds to an arc distance of ~0.15 o in 1 second  The CIDR are sensitive to smaller-scale structures  At 1 Hz: F-region structures (300 km) ~1570 m E-region structures (100 km) ~525 m  Limited by the Fresnel Scale F-region Fresnel Scale ~ 774.5 m E-region Fresnel Scale ~ 447.2 m 

9 ARL Applied Research Laboratories The University of Texas at Austin Features of UHF/VHF Beacon Electron Content Measurements  Spacecraft cross the field of view in ~20 min (GPS spacecraft take ~8hrs)  Enable tomographic reconstruction  Measurements from LEO spacecraft (~1000 km)  Purely ionospheric measurement  Shorter frequencies (400 MHz vrs 1575.42 MHz)  More precise TEC measurements  TEC ~  /f 2  CIDR ~ 15.5 more precise than GPS

10 ARL Applied Research Laboratories The University of Texas at Austin More Differences Between GPS and CIDRs  Tend to have a higher data rates  1 kHz decimated to 1-10 Hz  Allows measurements of the rapid ionospheric variations  Relative TEC measurements  Relative to an unknown integration constant  GPS TEC relative unknown transmitter and receiver biases

11 ARL Applied Research Laboratories The University of Texas at Austin CIDR Data Chain  Receiver records the raw Doppler measurements  Postprocessing code quality checks the Doppler measurements, calculates the positioning solutions, and converts the Doppler measurements to  TEC/  t and TEC

12 Sample Doppler File # 2629.864331.31780.83 # 1907188510Operational1 # 2008 299 17 33 36.000000 # 2008 299 17 48 21.000000 63216.19710.06377.1013197.6597.52226.836542.449797.69498.127 63217.19710.06587.1007397.42697.47926.842242.442297.58197.832 63218.19710.0687.1008597.87897.81226.847942.368397.69197.24 63219.19710.07017.2755897.55797.38926.853641.903797.65398.373 63220.19710.07227.9377598.10398.18926.859340.124697.44697.387 63221.19710.07448.1000197.43898.37226.86537.94298.40797.116 63222.19710.07658.1674197.46697.79726.870835.696797.71897.86 63223.19710.07878.2462498.14197.94926.876633.39397.70196.813 63224.19710.08098.3211698.0497.626.882431.64497.52998.165 63225.19710.08318.3949898.11498.02426.888231.394497.26397.765 63226.19710.08528.4651497.79797.826.89431.22397.79897.526 63227.19710.08758.5430897.43698.12126.899931.054598.3397.998 63228.19710.08978.6200297.74896.93826.905830.880997.91998.108 63229.19710.09198.7021798.11397.2526.911730.707597.74397.568 63230.19710.09418.7795497.85298.08226.917630.529497.08298.004 63231.19710.09638.8559997.78297.56926.923530.347797.38497.839 63232.19710.09868.9295998.00898.51826.929530.165597.24497.611 63233.19710.10089.0029697.70197.96926.935530.003198.07497.477 63234.19710.10319.0825198.25596.87126.941529.827497.15897.812 63235.19710.10539.1626897.10298.32326.947529.647697.73798.143 63236.19710.10769.2354197.40598.08126.953629.467697.75397.742 63237.19710.10999.3123297.26997.46126.959729.292197.72797.911 63238.19710.11229.3898797.55797.73326.965829.123697.73497.076 63239.19710.11459.4673297.84398.63926.971928.963196.9897.191

13 Sample Processed Text File # GLOBAL ATTRIBUTES -- name : value CONTACT : Trevor Garner, ARL:UT, garner@arlut.utexas.edu CREATOR : Kanish Mehta SOURCE : Applied Research Laboratories: University of Texas at Austin instrument : ARL:UT CIDR Receiver # 26 receiver_location : Helwan receiver_latitude : 29.8643 receiver_longitude : 31.317 receiver_altitude : 80.83 sample_rate_hz : 1 satellite_name : OSCAR 32 num_data : 643 # UT Relative TEC Rate Sat.Lat Sat.Lon Sat.Alt Azimuth Elevation F Lat F Long E Lat E Lon Phase Rate Phase Rate Sat.Vel Good # (sec) TEC (TECU) (TECU/1.00s) (deg) (deg) (km) (deg) (deg) (deg) (deg) (deg) (deg) VHF (Hz) UHF (Hz) (km/s) Flag 63278.2 3.0654 -0.0308161 52.2703 61.5188 1299.31 36.0752 2.37675 41.4956 43.0712 35.797 36.7374 10.6 27.5 20.5309 1 63279.2 3.07675 0.0113533 52.217 61.514 1299.23 36.1573 2.4098 41.4602 43.0659 35.7708 36.7281 10.2 27.5 20.6618 1 63280.2 3.07026 -0.00648761 52.1636 61.5092 1299.16 36.2396 2.44283 41.4248 43.0606 35.7447 36.7189 10.4 27.5 20.5964 1 63281.2 3.07675 0.00648761 52.1103 61.5044 1299.09 36.322 2.47583 41.3895 43.0553 35.7187 36.7097 10.3 27.7 20.8036 1 63282.2 3.04269 -0.0340599 52.0569 61.4996 1299.01 36.4045 2.50881 41.3542 43.05 35.6928 36.7005 10.5 27.4 20.4764 1 63283.2 3.04755 0.00486571 52.0036 61.4948 1298.94 36.4872 2.54178 41.319 43.0447 35.6671 36.6914 10.3 27.4 20.5418 1 63284.2 3.03458 -0.0129752 51.9502 61.4901 1298.86 36.5701 2.57472 41.2839 43.0394 35.6414 36.6823 10.4 27.4 20.5091 1 63285.2 3.05242 0.0178409 51.8969 61.4853 1298.79 36.6531 2.60763 41.2489 43.0341 35.6159 36.6732 10.2 27.5 20.6618 1 63286.2 3.04431 -0.00810951 51.8435 61.4805 1298.71 36.7362 2.64053 41.2139 43.0288 35.5904 36.6642 10.4 27.5 20.5964 1 63287.2 3.0362 -0.00810951 51.7902 61.4757 1298.64 36.8195 2.6734 41.1789 43.0236 35.5651 36.6552 10.4 27.5 20.5964 1 63288.2 3.04593 0.00973141 51.7368 61.4709 1298.56 36.9029 2.70625 41.1441 43.0183 35.5399 36.6462 10.2 27.5 20.6618 1 63289.2 3.02971 -0.016219 51.6835 61.4662 1298.49 36.9865 2.73908 41.1092 43.0131 35.5148 36.6373 10.4 27.4 20.5091 1 63290.2 3.02323 -0.00648761 51.6301 61.4614 1298.41 37.0702 2.77188 41.0745 43.0079 35.4898 36.6285 10.4 27.5 20.5964 1 63291.2 3.0216 -0.0016219 51.5768 61.4566 1298.34 37.1541 2.80466 41.0398 43.0026 35.465 36.6196 10.3 27.5 20.6291 1 63292.2 3.02971 0.00810951 51.5234 61.4518 1298.26 37.2381 2.83741 41.0052 42.9974 35.4402 36.6108 10.2 27.5 20.6618 1 63293.2 3.0216 -0.00810951 51.4701 61.4471 1298.18 37.3223 2.87015 40.9706 42.9922 35.4155 36.602 10.4 27.5 20.5964 1 63294.2 3.00538 -0.016219 51.4167 61.4423 1298.11 37.4066 2.90285 40.9362 42.9871 35.391 36.5933 10.4 27.4 20.5091 1 63295.2 2.99565 -0.00973141 51.3633 61.4375 1298.03 37.491 2.93553 40.9017 42.9819 35.3665 36.5846 10.4 27.6 20.6836 1 63296.2 2.9989 0.0032438 51.31 61.4328 1297.96 37.5757 2.96819 40.8674 42.9767 35.3422 36.576 10.2 27.3 20.4873 1 63297.2 2.98268 -0.016219 51.2566 61.428 1297.88 37.6604 3.00082 40.8331 42.9716 35.318 36.5674 10.4 27.4 20.5091 1 63298.2 2.96808 -0.0145971 51.2033 61.4232 1297.8 37.7453 3.03343 40.7988 42.9664 35.2938 36.5588 10.4 27.4 20.5091 1 63299.2 2.95511 -0.0129752 51.1499 61.4185 1297.73 37.8304 3.06601 40.7646 42.9613 35.2698 36.5503 10.4 27.4 20.5091 1 63300.2 2.94862 -0.00648761 51.0965 61.4137 1297.65 37.9156 3.09856 40.7305 42.9562 35.2459 36.5418 10.3 27.4 20.5418 1 63301.2 2.93564 -0.0129752 51.0432 61.4089 1297.57 38.0009 3.13109 40.6965 42.9511 35.2221 36.5333 10.4 27.5 20.5964 1 63302.2 2.92916 -0.00648761 50.9898 61.4042 1297.5 38.0864 3.1636 40.6625 42.946 35.1984 36.5249 10.3 27.4 20.5418 1 63303.2 2.91131 -0.0178409 50.9364 61.3994 1297.42 38.1721 3.19607 40.6285 42.9409 35.1748 36.5165 10.4 27.3 20.4218 1 63304.2 2.90483 -0.00648761 50.883 61.3947 1297.34 38.2579 3.22852 40.5947 42.9358 35.1513 36.5081 10.3 27.3 20.4545 1 63305.2 2.89672 -0.00810951 50.8297 61.3899 1297.26 38.3438 3.26094 40.5609 42.9308 35.1279 36.4998 10.3 27.3 20.4545 1

14 ARL Applied Research Laboratories The University of Texas at Austin Sample ITNE Observation

15 ARL Applied Research Laboratories The University of Texas at Austin ITNE Science Goals  Large-scale plasma structures  Chain is located underneath of equatorial fountain peaks (15.6 to 23.8 deg magnetic latitude)  Routine observations of the equatorial fountain peaks  Tomography and data assimilative reconstructions of the fountain  Small-scale plasma irregularities  TEC variations associated with equatorial anomaly peaks  Examine the consequence with tropospheric weather  Comparison with the American sector CIDR chain  Examine the impact of greater geographic/magnetic latitude offsets in the Americas

16 ARL Applied Research Laboratories The University of Texas at Austin Analysis of Sample Observation

17 Ionospheric Tomography  Traditional usage of the CIDR-like measurements  Utilizes crossing ray paths  Typically 3-5 receivers along aligned with the orbit  Assumes a slowly varying ionosphere  Typically 15 minute time steps

18 ARL Applied Research Laboratories The University of Texas at Austin Contact Information  If you are interested in working with ITNE data, please contact:  Ayman Mahrous (ayman.mahrous@gmail.com)  Trevor Garner (garner@arlut.utexas.edu)

19 ARL Applied Research Laboratories The University of Texas at Austin Summary  First ITNE CIDR is up and running  First results of Coherent Ionospheric Doppler Receiver measurements over Egypt, Mahrous, A., A. Shimeis, and T. Garner, Space Weather, 8, doi:10.1029/2009SW000548, 2010.  Excellent opportunity to study the northern crest of equatorial fountain in Africa  Please contact garner@arlut.utexas.edu or ayman.mahrous@gmail.com if you think ITNE data can help in your data study.


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