Media responsible for Faraday rotation: A review

Radio Science

Volumn 47, Issue 6, 2012, Pages

  Oberoi, D ^a,b   Lonsdale, C J ^a  

^a MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^b NATIONAL CENTRE FOR RADIO ASTROPHYSICS   (India)

Author keywords

[No Author keywords available]

Indexed keywords

HELIOSPHERES; HIGH SENSITIVITY MEASUREMENT; LONG WAVELENGTH; MAGNETIZED PLASMAS; PLASMASPHERE; RADIO FREQUENCIES; SCIENTIFIC OBJECTIVES; SPATIAL AND TEMPORAL VARIATION; TECHNOLOGICAL ADVANCES; WIDE FIELD-OF-VIEW;

CALIBRATION; MAGNETOSPHERE; RADIO ASTRONOMY;

IONOSPHERE;

EID: 84869382053     PISSN: 00486604     EISSN: None     Source Type: Journal    
DOI: 10.1029/2012RS004992     Document Type: Review

References (75)

1. Balogh, A., J. T. Gosling, J. R. Jokipii, R. Kallenbach, and H. Kunow (1999), Corotating Interaction Regions: Proceedings of an ISSI Workshop, 6-13 June 1998, Bern, Switzerland, Kluwer Acad., Dordrecht, Netherlands.
2. Bartels, J., N. H. Heck, and H. F. Johnston (1939), The three-hour index measuring geomagnetic activity, Terr. Magn. Atmos. Electr., 44, 411-454, doi:10.1029/TE044i004p00411.
3. Basu, S., S. Basu, J. Aarons, J. P. McClure, and M. D. Cousins (1978), On the coexistence of kilometer-and meter-scale irregularities in the nighttime equatorial F region, J. Geophys. Res., 83, 4219-4226, doi:10.1029/ JA083iA09p04219. (Pubitemid 9398989)
4. Bilitza, D. (2001), IRI 2000, Radio Sci., 36, 261-276, doi:10.1029/2000RS002432. (Pubitemid 32432667)
5. Bird, M. K. (2007), Coronal Faraday rotationof occulted radio signals, Astron. Astrophys. Trans., 26, 441-453, doi:10.1080/10556790701595236.
6. Bird, M. K., and P. Edenhofer (1990), Remote sensing observations of the solar corona, in Physics of the Inner Heliosphere, pp. 13-97, Springer, Berlin.
7. Bird, M. K., et al. (1985), White-light and radio sounding observations of coronal transients, Sol. Phys., 98, 341-368, doi:10.1007/BF00152465.
8. Bowman, J. D., and A. E. E. Rogers (2010), A lower limit of Dz > 0.06 for the duration of the reionization epoch, Nature, 468, 796-798, doi:10.1038/nature09601.
9. Breen, A. R., P. J. Moran, C. A. Varley, P. J. S. Williams, W. A. Coles, R. R. Grall, M. T. Klinglesmith, and J. Markkanen (1997), EISCAT measurements of interaction regions in the solar wind, Adv. Space Res., 20, 27-30, doi:10.1016/S0273-1177(97)00475-4.
10. Cahill, L. J., and P. G. Amazeen (1963), The boundary of the geomagnetic field, J. Geophys. Res., 68, 1835-1843, doi:10.1029/JZ068i007p01835.
11. Costain, C. H. (1960), The spectrum of the galactic radio emission, Mon. Not. R. Astron. Soc., 120, 248-312.
12. Coster, A. J., J. Foster, and P. J. Erickson (2003), Monitoring the ionosphere with GPS, GPS World, 14, 40-45.
13. Courtillot, V., and J. L. Le Mouel (1988), Time variations of the Earth's magnetic field-From daily to secular, Annu. Rev. Earth Planet. Sci., 16, 389-476, doi:10.1146/annurev.ea.16.050188.002133.
14. Crooker, N. U., et al. (1999), CIR morphology, turbulence, discontinuities, and energetic particles, Space Sci. Rev., 89, 179-220, doi:10.1023/A:1005253526438.
15. de Bruyn, A. G., P. Katgert, M. Haverkorn, and D. H. F. M. Schnitzeler (2006), Radio polarization and RM structure at high Galactic latitudes, Astron. Nachr., 327, 487-490, doi:10.1002/asna.200610566. (Pubitemid 44076617)
16. de Oliveira-Costa, A., M. Tegmark, B. M. Gaensler, J. Jonas, T. L. Landecker, and P. Reich (2008), A model of diffuse Galactic radio emission from 10 MHz to 100 GHz, Mon. Not. R. Astron. Soc., 388, 247-260, doi:10.1111/j.1365- 2966.2008.13376.x.
17. de Vos, M., A. W. Gunst, and R. Nijboer (2009), The LOFAR telescope: System architecture and signal processing, Proc. IEEE, 97, 1431-1437, doi:10.1109/JPROC.2009.2020509.
18. Ellingson, S. W., T. E. Clarke, A. Cohen, J. Craig, N. E. Kassim, Y. Pihlstrom, L. J. Rickard, and G. B. Taylor (2009), The long wavelength array, Proc. IEEE, 97, 1421-1430, doi:10.1109/JPROC.2009.2015683.
19. Escoubet, C. P., A. Pedersen, R. Schmidt, and P. A. Lindqvist (1997), Density in the magnetosphere inferred from ISEE 1 spacecraft potential, J. Geophys. Res., 102, 17,595-17,609, doi:10.1029/97JA00290. (Pubitemid 127694747)
20. Finlay, C. C., et al. (2010), International Geomagnetic Reference Field: The eleventh generation, Geophys. J. Int., 183, 1216-1230, doi:10.1111/j.1365- 246X.2010.04804.x.
21. Gallagher, D. L., P. D. Craven, and R. H. Comfort (2000), Global core plasma model, J. Geophys. Res., 105, 18,819-18,834, doi:10.1029/1999JA000241.
22. Hargreaves, J. K. (1992), The Solar-Terrestrial Environment: An Introduction to Geospace-The Science of the Terrestrial Upper Atmosphere, Ionosphere and Magnetosphere, Cambridge Univ. Press, Cambridge, U. K.
23. Haslam, C. G. T., C. J. Salter, H. Stoffel, and W. E. Wilson (1982), A 408 MHz all-sky continuum survey. II-The atlas of contour maps, Astron. Astrophys. Suppl. Ser., 47, 1-143.
24. Haverkorn, M., P. Katgert, and A. G. de Bruyn (2000), Structure in the local Galactic ISM on scales down to 1 pc, from multi-band radio polarization observations, Astron. Astrophys., 356, L13-L16.
25. Haverkorn, M., P. Katgert, and A. G. de Bruyn (2003a), Characteristics of the structure in the Galactic polarized radio background at 350 MHz, Astron. Astrophys., 403, 1045-1057, doi:10.1051/0004-6361:20030464.
26. Haverkorn, M., P. Katgert, and A. G. de Bruyn (2003b), Multi-frequency polarimetry of the Galactic radio background around 350 MHz. II. A region in Horologium around l = 137degr, b = 7degr, Astron. Astrophys., 404, 233-247, doi:10.1051/0004-6361:20030530.
27. Haverkorn, M., P. Katgert, and A. G. de Bruyn (2003c), Multi-frequency polarimetry of the Galactic radio background around 350 MHz. I. A region in Auriga around l = 161 deg, b = 16 deg, Astron. Astrophys., 403, 1031-1044, doi:10.1051/0004-6361:20030432.
28. Hayashi, H., N. Nishitani, T. Ogawa, Y. Otsuka, T. Tsugawa, K. Hosokawa, and A. Saito (2010), Large-scale traveling ionospheric disturbance observed by superDARN Hokkaido HF radar and GPS networks on 15 December 2006, J. Geophys. Res., 115, A06309, doi:10.1029/2009JA014297.
29. Hernández-Pajares, M., J. M. Juan, and J. Sanz (2006), Medium-scale traveling ionospheric disturbances affecting GPS measurements: Spatial and temporal analysis, J. Geophys. Res., 111, A07S11, doi:10.1029/2005JA011474.
30. Hoogeveen, G. W., and A. R. Jacobson (1997), Radio interferometer measurements of plasmasphere density structures during geomagnetic storms, J. Geophys. Res., 102, 14,177-14,188, doi:10.1029/97JA00484. (Pubitemid 127694391)
31. Huang, Y.-N. (1978), Solar cycle variation in the total electron content at Sagamore Hill, J. Atmos. Terr. Phys., 40, 733-739.
32. Hunsucker, R. D., and J. K. Hargreaves (1988), A study of gravity waves ionospheric electron content at L = 4, J. Atmos. Terr. Phys., 50, 167-172.
33. Hysell, D. L., and J. D. Burcham (2002), Long term studies of equatorial spread/F using the JULIA radar at Jicamarca, J. Atmos. Sol. Terr. Phys., 64, 1531-1543, doi:10.1016/S1364-6826(02)00091-3. (Pubitemid 35016250)
34. Ingleby, L. D., S. R. Spangler, and C. A. Whiting (2007), Probing the large-scale plasma structure of the solar corona with Faraday rotation measurements, Astrophys. J., 668, 520-532, doi:10.1086/521140.
35. Jacobson, A. R., R. C. Carlos, R. S. Massey, and G. Wu (1995), Observations of traveling ionospheric disturbances with a satellite-beacon radio interferometer: Seasonal and local time behavior, J. Geophys. Res., 100, 1653-1665, doi:10.1029/94JA02663.
36. Jacobson, A. R., G. Hoogeveen, R. C. Carlos, G. Wu, B. G. Fejer, and M. C. Kelley (1996), Observations of inner plasmasphere irregularities with a satellite-beacon radio-interferometer array, J. Geophys. Res., 101, 19,665-19,682, doi:10.1029/96JA01253.
37. Jansky, K. G. (1932), Directional studies of atmospherics at high frequencies, Proc. Inst. Radio Eng., 20, 1920-1932.
38. Jelic, V., S. Zaroubi, P. Labropoulos, G. Bernardi, A. G. de Bruyn, and L. V. E. Koopmans (2010), Realistic simulations of the Galactic polarized foreground: consequences for 21-cm reionization detection experiments, Mon. Not. R. Astron. Soc., 409, 1647-1659, doi:10.1111/j.1365-2966. 2010.17407.x.
39. Jensen, E. A., P. P. Hick, M. M. Bisi, B. V. Jackson, J. Clover, and T. Mulligan (2010), Faraday rotation response to coronal mass ejection structure, Sol. Phys., 265, 31-48, doi:10.1007/s11207-010-9543-2.
40. Johnston, S., A. Karastergiou, D. Mitra, and Y. Gupta (2008), Multifre-quency integrated profiles of pulsars, Mon. Not. R. Astron. Soc., 388, 261-274, doi:10.1111/j.1365-2966.2008.13379.x.
41. Kelley, M. C., R. C. Livingston, C. L. Rino, and R. T. Tsunoda (1982), The vertical wave number spectrum of topside equatorial spread F: Estimates of backscatter levels and implications for a unified theory, J. Geophys. Res., 87, 5217-5221, doi:10.1029/JA087iA07p05217.
42. Kirkland, M. W., and A. R. Jacobson (1998), Drift-parallax determination of the altitude of traveling ionospheric disturbances observed with the Los Alamos radio-beacon interferometer, Radio Sci., 33, 1807-1826, doi:10.1029/98RS02033.
43. Ko, H. C., and J. D. Kraus (1956), A new radio map of the sky and a model of the galaxy, Astron. J., 61, 182, doi:10.1086/107391.
44. Kotake, N., Y. Otsuka, T. Tsugawa, T. Ogawa, and A. Saito (2006), Clima-tological study of GPS total electron content variations caused by medium-scale traveling ionospheric disturbances, J. Geophys. Res., 111, A04306, doi:10.1029/2005JA011418.
45. Kotake, N., Y. Otsuka, T. Ogawa, T. Tsugawa, and A. Saito (2007), Statistical study of medium-scale traveling ionospheric disturbances observed with the GPS networks in Southern California, Earth Planets Space, 59, 95-102. (Pubitemid 46614186)
46. Lawrence, R. S., C. G. Little, and H. J. A. Chivers (1964), A survey of ionospheric effects upon Earth-space radio propagation, Proc. IEEE, 45, 4-27.
47. Levy, G. S., T. Sato, B. L. Seidel, C. T. Stelzried, J. E. Ohlson, and W. V. T. Rusch (1969), Pioneer 6: Measurement of transient Faraday rotation phenomena observed during solar occultation, Science, 166, 596-598, doi:10.1126/science.166.3905.596.
48. Liu, Y., W. B. Manchester, IV, J. C. Kasper, J. D. Richardson, and J. W. Belcher (2007), Determining the magnetic field orientation of coronal mass ejections from Faraday rotation, Astrophys. J., 665, 1439-1447, doi:10.1086/520038.
49. Lonsdale, C. J., et al. (2009), The Murchison Widefield Array: Design overview, Proc. IEEE, 97, 1497-1506, doi:10.1109/JPROC.2009.2017564.
50. Manchester, R. N. (1971), Observations of pulsar polarization at 410 and 1665 MHz, Astrophys. J. Suppl. Ser., 23, 283-319, doi:10.1086/190240.
51. Mancuso, S., and S. R. Spangler (2000), Faraday rotation and models for the plasma structure of the solar corona, Astrophys. J., 539, 480-491, doi:10.1086/309205.
52. Manoharan, P. K. (2010), Ooty Interplanetary Scintillation-Remote-sensing observations and analysis of coronal mass ejections in the helio-sphere, Sol. Phys., 265, 137-157, doi:10.1007/s11207-010-9593-5.
53. Muller, C. A. (1963), Galactic background polarization at 610 Mc/s, Nature, 200, 155-156, doi:10.1038/200155a0.
54. Ness, N. F. (1969), The geomagnetic tail., Rev. Geophys., 7, 97-127, doi:10.1029/RG007i001p00097.
55. Parsons, A. R., et al. (2010), The precision array for probing the epoch of re-ionization: Eight station results, Astron. J., 139, 1468-1480, doi:10.1088/0004-6256/139/4/1468.
56. Pen, U.-L., T.-C. Chang, C. M. Hirata, J. B. Peterson, J. Roy, Y. Gupta, J. Odegova, and K. Sigurdson (2009), The GMRT EoR experiment: Limits on polarized sky brightness at 150 MHz, Mon. Not. R. Astron. Soc., 399, 181-194, doi:10.1111/j.1365-2966.2009.14980.x.
57. Rideout, W., and A. J. Coster (2006), Automated GPS processing for global total electron content data, GPS Solutions, 10, 219-228, doi:10.1007/s10291- 006-0029-5.
58. Rishbeth, H., and M. Mendillo (2001), Patterns of F2-layer variability, J. Atmos. Sol. Terr. Phys., 63, 1661-1680, doi:10.1016/S1364-6826(01) 00036-0.
59. Rogers, A. E. E., and J. D. Bowman (2008), Spectral index of the diffuse radio background measured from 100 to 200 MHz, Astron. J., 136, 641-648, doi:10.1088/0004-6256/136/2/641.
60. Sakurai, T., and S. R. Spangler (1994), Use of the very large array for measurement of time variable Faraday rotation, Radio Sci., 29, 635-662, doi:10.1029/94RS00330.
61. Salah, J. E., C. J. Lonsdale, D. Oberoi, R. J. Cappallo, and J. C. Kasper (2005), Space weather capabilities of low frequency radio arrays, in Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, vol. 5901, edited by S. Fineschi and R. A. Viereck, pp. 124-134, Bellingham, Wash., doi:10.1117/12.613448. (Pubitemid 43039221)
62. Singh, S., D. K. Bamgboye, J. P. McClure, and F. S. Johnson (1997), Morphology of equatorial plasma bubbles, J. Geophys. Res., 102, 20,019-20,029, doi:10.1029/97JA01724. (Pubitemid 127694777)
63. Smirnova, T. V., I. V. Chashei, and V. I. Shishov (2009), Radio sounding of the circumsolar plasma using polarized pulsar pulses, Astron. Rep., 53, 252-261, doi:10.1134/S106377290903007X.
64. Spangler, S. R. (2005), The strength and structure of the coronal magnetic field, Space Sci. Rev., 121, 189-200, doi:10.1007/s11214-006-4719-7. (Pubitemid 43839014)
65. Spangler, S. R., and C. A. Whiting (2009), Radio remote sensing of the corona and the solar wind, in Universal Heliophysical Processes, Proceedings of the International Astronomical Union, IAU Symposium, vol. 257, edited by N. Gopalswamy and D. F. Webb, pp. 529-541, Cambridge Univ. Press, Cambridge, U. K., doi:10.1017/S1743921309029834.
66. St. Cyr, O. C., J. T. Burkepile, A. J. Hundhausen, and A. R. Lecinski (1999), A comparison of ground-based and spacecraft observations of coronal mass ejections from 1980-1989, J. Geophys. Res., 104, 12,493-12,506, doi:10.1029/1999JA900045.
67. Taylor, A. R., J. M. Stil, and C. Sunstrum (2009), A rotation measure image of the sky, Astrophys. J., 702, 1230-1236, doi:10.1088/0004-637X/702/2/ 1230.
68. Tingay, S. J., et al. (2012), The Murchison Widefield Array: The square kilometre array precursor at low radio frequencies, Publ. Astron. Soc. Aust., in press.
69. Tsugawa, T., A. Saito, and Y. Otsuka (2004), A statistical study of large-scale traveling ionospheric disturbances using the GPS network in Japan, J. Geophys. Res., 109, A06302, doi:10.1029/2003JA010302.
70. Tsugawa, T., K. Shiokawa, Y. Otsuka, T. Ogawa, A. Saito, and M. Nishioka (2006), Geomagnetic conjugate observations of large-scale traveling ionospheric disturbances using GPS networks in Japan and Australia, J. Geophys. Res., 111, A02302, doi:10.1029/2005JA011300.
71. Tsugawa, T., Y. Otsuka, A. J. Coster, and A. Saito (2007), Medium-scale traveling ionospheric disturbances detected with dense and wide TEC maps over North America, Geophys. Res. Lett., 34, L22101, doi:10.1029/2007GL031663. (Pubitemid 351222775)
72. Tsunoda, R. T. (1980), Magnetic-field-aligned characteristics of plasma bubbles in the nighttime equatorial ionosphere, J. Atmos. Terr. Phys., 42, 743-752.
73. Valladares, C., J. Villalobos, R. Sheehan, and M. Hagan (2004), Latitudinal extension of low-latitude scintillations measured with a network of GPS receivers, Ann. Geophys., 22, 3155-3175, doi:10.5194/angeo-22-3155-2004. (Pubitemid 39437265)
74. Wieringa, M. H., A. G. de Bruyn, D. Jansen, W. N. Brouw, and P. Katgert (1993), Small scale polarization structure in the diffuse galactic emission at 325 MHz, Astron. Astrophys., 268, 215-229.
75. Wijnholds, S., S. van der Tol, R. Nijboer, and A.-J. van der Veen (2010), Calibration challenges for future radio telescopes, IEEE Signal Process. Mag., 27, 30-42, doi:10.1109/MSP.2009.934853.