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Интеллектуальная Система Тематического Исследования НАукометрических данных |
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The Potential for a Ka-band (32 GHz) Worldwide VLBI Networkдоклад на конференции
- Авторы: Jacobs Christopher S., Zharov V., Colomer F., García-Miró C., Gómez-González J., Gulyaev S., Horiuchi S., Ichikawa R., Kraus A., Kronschnabl G., López-Fernández J.A., Lovell J., Natusch T., Neidhardt A., Phillips C., Porcas R., Romero-Wolf A., Saldana L., Schreiber U., Sotuela I., Takeuchi H., Trinh J., Tzioumis A., de Vicente P., Bach U.
- Конференция : IVS 2012 General Meeting
- Даты проведения конференции: 2012
- Тип доклада: не указан
- Докладчик: не указан
- Место проведения: Madrid, Spain, Spain
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Аннотация доклада:
Ka-band (32 GHz, 9 mm) Very Long Baseline Interferometric (VLBI) networking has now begun and has tremendous potential for expansion over the next few years. Ka-band VLBI astrometry from NASA's Deep Space Network has already developed a catalog of ∼470 observable sources with highly accurate positions. Now, several antennas worldwide are planning or are considering adding Ka-band VLBI capability. Thus, there is now an opportunity to create a worldwide Ka-band network with potential for high resolution imaging and astrometry. With baselines approaching a Giga-lambda, a Ka-band network would be able to probe source structure at the nano-radian (200 μas) level (100X better than Hubble) and thus gain insight into the astrophysics of the most compact regions of emission in active galactic nuclei. We discuss the advantages of Ka-band, show the known sources and candidates, simulate projected baseline (uv) coverage, and discuss potential radio frequency feeds
- Добавил в систему: Жаров Владимир Евгеньевич