Synchrotron Spectral Curvature from 22 MHZ to 23 GHZ

机译：从22 MHZ到23 GHZ的同步加速器光谱曲率

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We combine surveys of the radio sky at frequencies 22 MHz to 1.4 GHz with data from the ARCADE-2 instrument at frequencies 3 GHz to 10 GHz to characterize the frequency spectrum of diffuse synchrotron emission in the Galaxy. The radio spectrum steepens with frequency from 22 MHz to 10 GHz. The projected spectral index at 23 GHz derived from the low-frequency data agrees well with independent measurements using only data at frequencies 23 GHz and above. Comparing the spectral index at 23 GHz to the value from previously published analyses allows extension of the model to higher frequencies. The combined data are consistent with a power-law index beta = -2.64 +/-= 0.03 at 0.31 GHz, steepening by an amount of Delta-beta = 0.07 every octave in frequency. Comparison of the radio data to models including the cosmic-ray energy spectrum suggests that any break in the synchrotron spectrum must occur at frequencies above 23 GHz.

机译：我们将22 MHz至1.4 GHz频率的无线电天空的测量结果与3 GHz至10 GHz频率的ARCADE-2仪器的数据相结合，以表征银河系中散射同步加速器发射的频谱。无线电频谱的频率从22 MHz到10 GHz变陡。从低频数据得出的在23 GHz时的投影光谱指数与仅使用23 GHz及以上频率的数据进行独立测量非常吻合。将23 GHz的频谱指数与先前发布的分析值进行比较，可以将模型扩展到更高的频率。合并后的数据在0.31 GHz时与幂律指数beta = -2.64 + /-= 0.03一致，在频率上每倍频程增加Delta-beta = 0.07。将无线电数据与包括宇宙射线能谱的模型进行比较表明，同步加速器谱中的任何破坏都必须发生在23 GHz以上的频率上。

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Kogut, Alan J.;
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年度 2012
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1. Evolutionary features of the variations in the fluxes of selected extragalactic radio sources at 102 MHz, 22 GHz and 36 GHz [J] . Alexandr Volvach, Michail Ryabov Astronomical and astrophysical transactions: The journal of the Soviet Astronomical Society . 2005,第5期

机译：选定的河外无线电源在102 MHz，22 GHz和36 GHz处通量变化的演变特征
2. 10-GHz Bandwidth RF Spectral Analyzer With MHz Resolution Based on Spectral Hole Burning in Tm~(3+):YAG [J] . G. Gorju, V. Crozatier, I. Lorgere, IEEE Photonics Technology Letters . 2005,第11期

机译：基于Tm〜（3 +）：YAG中光谱孔燃烧的MHz分辨率的10 GHz带宽RF光谱分析仪
3. A 5 GHz 0.5 V Hybrid Class-B/F−1 CMOS Oscillator With −147 dBc/Hz Phase Noise at 10 MHz Offset Using Body-Biased 22 nm FDSOI [J] . El-Aassar Omar, Rebeiz Gabriel M. IEEE microwave and wireless components letters . 2020,第10期

机译：5 GHz 0.5 V混合体-B / F-1 CMOS振荡器，具有-147 dBc / Hz相位噪声，使用Body-Biased22 NM FDSOI偏移10 MHz
4. 71–95 GHz (23–40 PAE) and 96–120 GHz (19–22 PAE) high efficiency 100–130 mW power amplifiers in InP HBT [C] . Zach Griffith, Miguel Urteaga, Petra Rowell, IEEE MTT-S International Microwave Symposium . 2016

机译：InP HBT中的71–95 GHz（23–40％PAE）和96–120 GHz（19–22％PAE）高效100–130 mW功率放大器
5. I. A 22 GHz VLBI survey of 140 compact extragalactic radio sources. II. VLBA polarization observations of gamma-ray blazars at 15 and 22 GHz. [D] . Moellenbrock, George A., III. 1999

机译：I.对140个紧凑型河外无线电源进行的22 GHz VLBI调查。二。在15 GHz和22 GHz的伽玛射线暴的VLBA极化观测。
6. Radiation Characterization of an Intra-Oral Wireless Device at Multiple ISM Bands: 433 MHz 915 MHz and 2.42 GHz [O] . Xueliang Huo, Uei-Ming Jow, Maysam Ghovanloo -1

机译：在多个Ism频段的口腔内的无线设备的辐射特性：433兆赫915兆赫和2.42 GHz的
7. Flux density monitoring of extragalactic radio sources. Observations at 22, 37 GHz and 102 MHz within the research programs for the RT-22 CrAO and the Odesa Observatory "URAN-4" IRA NASU [O] . Volvach A.E., Ryabov M.I. 2005

机译：河外无线电源的通量密度监视。在RT-22 CrAO和Odesa天文台“ URAN-4” IRA NASU的研究计划中以22、37 GHz和102 MHz进行的观测
8. Synchrotron Spectral Curvature from 22 MHZ to 23 GHZ. [R] . Kogut, A. J. 2012

机译：同步加速器光谱曲率从22 mHZ到23 GHZ。

Synchrotron Spectral Curvature from 22 MHZ to 23 GHZ

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