Slant path 30 to 12.5 GHz copolar phase difference, first results from measurements using the Olympus satellite

Access Full Text

Slant path 30 to 12.5 GHz copolar phase difference, first results from measurements using the Olympus satellite

For access to this article, please select a purchase option:

Buy article PDF
£12.50
(plus tax if applicable)
Buy Knowledge Pack
10 articles for £75.00
(plus taxes if applicable)

IET members benefit from discounts to all IET publications and free access to E&T Magazine. If you are an IET member, log in to your account and the discounts will automatically be applied.

Learn more about IET membership 

Recommend Title Publication to library

You must fill out fields marked with: *

Librarian details
Name:*
Email:*
Your details
Name:*
Email:*
Department:*
Why are you recommending this title?
Select reason:
 
 
 
 
 
Electronics Letters — Recommend this title to your library

Thank you

Your recommendation has been sent to your librarian.

The first results of 30 to 12.5 GHz copolar phase measurements using the propagation beacons of the Olympus satellite of ESA are presented. Examples of ionospheric and rain effects are given. The method of data processing is discussed.

Inspec keywords: ionospheric electromagnetic wave propagation; rain; microwave links; satellite links; tropospheric electromagnetic wave propagation; radiowave propagation

Other keywords: 30 to 12.5 GHz; rain effects; ESA; copolar phase difference; propagation beacons; copolar phase measurements; ionospheric effects; Olympus satellite; method of data processing; European Space Agency; SHF

Subjects: Satellite communication systems; Water in the atmosphere (humidity, clouds, evaporation, precipitation); Radiowave propagation; Electromagnetic wave propagation and interactions in the lower atmosphere; Ionospheric electromagnetic wave propagation

References

    1. 1)
      • J. Awaka , M. Fujita . Measurement of the total electron content by means of differential phase shift method using coherent SHF signals from a geostationary satellite. J. Atm. Terr. Phys. , 1441 - 1446
    2. 2)
      • A. Picquenard . (1974) , Radiowave propagation.
    3. 3)
      • Thompson, P., Dissanayake, A., Watson, P.: `The frequency dependence of microwave propagation through rainfall', AGARD Conf. Proc. 284, 1980, Wachtberg-Werthoven, .
    4. 4)
      • M. Kotaki , I. Kurigi , C. Katoh , H. Sugiuchi . Effects of the ionosphere on the radio horizon in HF band on the earth–space paths. J. Radio Research Laboratories , 133 - 148
    5. 5)
      • `Atlas of ionospheric characteristics', Report 340, 1966.
http://iet.metastore.ingenta.com/content/journals/10.1049/el_19900736
Loading

Related content

content/journals/10.1049/el_19900736
pub_keyword,iet_inspecKeyword,pub_concept
6
6
Loading