Results of foF2 data testing with the undiv program

Studia Geophysica et Geodaetica

Volumn 41, Issue 1, 1997, Pages 82-87

  Burešová, Dalia ^a,b  

^a INSTITUTE OF ATMOSPHERIC PHYSICS   (Czech Republic)

^b NONE   (Czech Republic)

Author keywords

Data testing; Ionosphere; Predictions

Indexed keywords

EID: 0009739423     PISSN: 00393169     EISSN: None     Source Type: Journal    
DOI: 10.1023/A:1023392808566     Document Type: Article

References (9)

1. Balan N., Bailey G J., Su Y Z., 1996: Variations of the ionosphere and related solar fluxes during solar cycles 21 and 22. Adv. Space Res. 18, No. 8, 11-14.
2. Bradley P. A., 1993: A study of the differences in foF2 and M(3000)F2 between solar cycles. Proceedings of the Graz Workshop, 2(1), 67-77.
3. Bradley P. A., Kouris S. S., Xenos Th. D., Dick M. I., 1995: Reference of foF2 measurement data set for long-term temperate-latitude regional mapping. Adv. Space Res. 16, No. 1, 163-166.
4. Dai Kailiang, Quan Kunhai, Liu Ruiyuan., 1993: Comparative study of modeled foF2 with observations in China. Proceedings of 1993 International Symposium on Radio Propagation (ISRP'93), Beijing, China.
5. Donnelly R. F., 1989: Solar UV variability. Handbook for MAP 29, 1-8.
6. Niberon M. F., 1994: PRIME data base for use in map generation and for testing maps. COST238TD(94)001.
7. Piggott W. R., Rawer K., 1972: URSI Handbook of Ionogram Interpretation and Reduction. WDC-A, Rep. UAG-23, Boulder.
8. PRIME Final Report, ed.Bradley P. A., ECSC-EEC-EAEC, Brussels, 1995.
9. Radicella S. M., 1996 : private communication.