KVN and VERA Array

Beam pattern and size

Figure 4 show the beam patterns in the K band. The side-lobe level is less than about -15 dB, except for the relatively high side-lobe level of about -10 dB for the separation angle of 2.0 deg at Ogasawara station. The side-lobe of the beam patterns has an asymmetric shape, but the main beam has a symmetric Gaussian shape without dependence on separation angle. The measured beam sizes (HPBW) in the K band and the Q band based on the data of the pointing calibration are also summarized in Table 4. The main beam sizes show no dependence on the dual-beam separation angle.

The optics of KVN antenna is a shaped Cassegrain type of which the main reflector and subreflector are shaped to have a uniform illumination pattern on an aperture plane. Because of the uniform illumination, KVN antennas can get higher aperture efficiency than value of typical Cassegrain type antenna. However, higher side-lobe level is inevitable. OTF images of Jupiter at K and Q bands are shown in Figure 4. The map size is 12' X 10' and the first side-lobe pattern is clearly visible. Typical side-lobe levels of KVN antennas are 13-14dB.

Figure 4:The beam patterns in the K-band for VERA (A-beam) Iriki with the separation angle of 0 (Upper left) and Ogasawara with the separation angle of 2.0(Upper right), and in K/Q-band for KVN Yonsei. The patterns of VERA antennas were derived from the mapping observation of strong HO maser toward W49N, which can be assumed as a point source, with grid spacing of . In the case of KVN antennas, the patterns were derived from the OTF images of Venus at K/Q-band.

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KaVA ( KVN and VERA Array )