TY - MGZN AU - Michael Lombardi AB -

Radio station WWV is known as a source of accurate time. However, since March 6, 1923, the original purpose of WWV has been to provide standard frequency signals, with signals broadcast in the LF and MF bands. As detailed in Hoy J. Walls’ “The Standard-Frequency Set at WWV” in the October 1924 issue of QST, this
was in the early days of broadcast radio, when having an accurate frequency reference was essential for keeping stations from interfering with each other. A century later, the standard frequency signals remain essential to radio broadcasters, calibration laboratories, space weather researchers, and radio amateurs.

BT - QST C1 -

This article is posted to hamsci.org with permission from the ARRL.

Full text: 2023-03 QST Lombardi.pdf

DA - 03/2023 IS - 3 LA - eng M1 - 3 N2 -

Radio station WWV is known as a source of accurate time. However, since March 6, 1923, the original purpose of WWV has been to provide standard frequency signals, with signals broadcast in the LF and MF bands. As detailed in Hoy J. Walls’ “The Standard-Frequency Set at WWV” in the October 1924 issue of QST, this
was in the early days of broadcast radio, when having an accurate frequency reference was essential for keeping stations from interfering with each other. A century later, the standard frequency signals remain essential to radio broadcasters, calibration laboratories, space weather researchers, and radio amateurs.

NV - 12 PY - 2023 SP - 33 EP - 37 T2 - QST TI - Measuring the Frequency Accuracy and Stability of WWV and WWVH VL - 107 SN - 0033-4812 ER -