  Mars Orbiter MAGnetometer (MOMAG) is a scientifc instrument onboard the
orbiter of China's first mission for Mars -- Tianwen-1. It started to routinely
measure the magnetic field from the solar wind to magnetic pile-up region
surrounding Mars since November 13, 2021. Here we present its in-flight
performance and first science results based on the first one and a half months'
data. By comparing with the magnetic field data in the solar wind from the Mars
Atmosphere and Volatile EvolutioN (MAVEN), the magnetic field by MOMAG is at
the same level in magnitude, and the same magnetic structures with the similar
variations in three components could be found in MOMAG data. In the first one
and a half months, we recognize 158 clear bow shock (BS) crossings from MOMAG
data, whose locations statistically match well with the modeled average BS. We
also identify 5 pairs of simultaneous BS crossings of the Tianwen-1's orbiter
and MAVEN. These BS crossings confirm the global shape of modeled BS as well as
the south-north asymmetry of the Martian BS. Two presented cases in this paper
suggest that the BS is probably more dynamic at flank than near the nose. So
far, MOMAG performs well, and provides accurate magnetic field vectors. MOMAG
is continuously scanning the magnetic field surrounding Mars. These
measurements complemented by observations from MAVEN will undoubtedly advance
our understanding of the plasma environment of Mars.
