Pulsar II manual 技術仕様

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Pulsar II・手入れと使用方法ガイド

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技術仕様

<タイプ:小型ダイアフラム・コンデンサー

<極性:カーディオイド

<周波数特性20Hz – 20kHz

<感度13.8 mV/Pa -37dBV ref. 1V/Pa

<最大 SPL <0.5%スレッショルド・レベル)134dB144dB SPL -10dBパッド)

<等価ノイズレベル15dB A-weighted

<出力インピーダンス300 - 600Ω

<推奨マイク・プリ入力インピーダンス1 – 2.5 kΩ

<プリアンプ・トポロジーClass A FET、変圧器不要

<電源条件30 VDC – 50 VDCファンタム電源

<端子3ピンXLR(オス)

<サイズ:直径22mm 0.87)、高さ132mm 5.20

<重量115 g 4.0 oz

M-Audio Pulsar IIマイクロフォンの周波数特性表:

80Hz

M-Audio Pulsar IIマイクロフォンの極性レスポンス表:

180°

150°

120°

90°

-20 dB -15 dB

60°-10 dB -5 dB

30°

+5 dB

日本語

150°

120°

90°

60°

30°

250Hz1000Hz

5000Hz 10000Hz

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Contents Pulsar はじめに 製品パッケージ内容カーディオイド・パターン 利用方法マイクロフォンの取り扱い 技術仕様 Jp/warrantyでご覧下さい。 製品保証Audio USA

II specifications

Pulsar II is an advanced, state-of-the-art astronomical instrument designed to push the boundaries of our understanding of the universe. This high-performance telescope represents the culmination of decades of research and innovation, harnessing cutting-edge technologies to provide unprecedented observational capabilities.

One of the distinguishing features of Pulsar II is its exceptionally large aperture, which allows it to capture light from some of the faintest celestial objects. This large collecting area, combined with a sophisticated light-gathering system, enables astronomers to observe distant galaxies, nebulae, and exoplanets with remarkable clarity. The telescope's ability to detect low-light emissions makes it invaluable for studying the early universe and the formation of cosmic structures.

The Pulsar II utilizes an array of advanced imaging technologies, including adaptive optics. This technology compensates for the distortion caused by Earth's atmosphere, providing sharper images and enhancing the telescope's resolution. Coupled with high-resolution cameras and spectrographs, Pulsar II can capture detailed spectra of celestial objects, allowing scientists to analyze their chemical compositions and velocities.

In addition to its optical capabilities, Pulsar II is equipped with multi-wavelength observation systems. This feature enables it to collect data across a broad range of the electromagnetic spectrum, from radio waves to gamma rays. By integrating information from diverse wavelengths, astronomers can gain a more comprehensive understanding of astronomical phenomena and their underlying processes.

Another significant characteristic of Pulsar II is its automated observational scheduling system. This innovative technology allows the telescope to autonomously identify targets of interest, optimize observation times, and adjust its settings based on real-time atmospheric conditions. As a result, Pulsar II maximizes its efficiency and productivity, capturing vast amounts of data for further analysis.

Furthermore, Pulsar II is built with a modular design, enabling it to be easily upgraded with the latest technologies as they become available. This adaptability ensures that the instrument remains at the forefront of astronomical research for years to come.

In summary, Pulsar II is a remarkable instrument that combines a large aperture, advanced imaging technologies, multi-wavelength capabilities, and automation to enhance our exploration of the universe. Its innovative features and characteristics set a new standard for modern astronomy, promising to unveil the mysteries of the cosmos in unprecedented detail.