The Schumann resonances (SR) are electromagnetic oscillations of the Earth-ionosphere cavity at frequencies of 7.8, 14, 20, 26, 33, 39, and 45 Hz. The long-term monitoring of the Schumann phenomenon has recently drawn attention, not least from the space-geophysics community [
1‐
3]. SR measurements and analysis provide information on the planetary thunderstorm activities, the properties of lower ionosphere layers, the Earth surface and atmosphere temperature variations, and the properties of earthquakes as well as on the studies of other celestial bodies [
4‐
9]. Consequently, increased interest has been shown by the scientific community on the methods and techniques employed in SR experimental detection. The detection of SR is a complex procedure that employs the limited energy generated and dissipated by the global lighting activity. This total energy is then smeared inside the huge volume of the Earth-ionosphere cavity, providing electric and magnetic field components. The prevailed electric component is vertically oriented, and the corresponding amplitude is close to 10
−7 V/m. The magnetic field exhibits two horizontally potential components at N-S and E-W orientation with amplitudes of few tenths of picotesla. The detection of such weak electromagnetic fields in noisy environments is too difficult. Additionally, hardware imperfections can significantly reduce the performance of the system [
10,
11]. To improve the signal-to-noise ratio (SNR), it is necessary to use specialized sensors and electronic equipment [
12]. Especially, in the ELF band, where Schumann resonances lie, very few works give details about measurement equipment used regarding electrical and magnetic antennas, the analog front-end, and the data acquisition module [
13]. In the observation system of ULF/ELF emissions at Nakatsugawa, the signal observed by the N-S sensor (each coil consists of perm alloy of 1.2 m long with 100,000 turns of the copper wire) is fed to a preamplifier, then to a low-pass filter of 10 and 30 Hz and main-amplifier, stored on DL-708 data recorder and saved on a hard disk. Summarized values of the induction coils, the amplification, and filtering are given for the observation system of ULF/ELF emissions at Nakatsugawa [
14]. Two research teams from Mexico have developed a Schumann resonance station with two inductive antennas. Details about the structure and development of the magnetic antenna are given. This station measures the first three harmonics [
15]. In SR observatories in southwestern China, the frequency band of the instruments is about 3–29 Hz (in the range of 3 dB), and the sampling frequency is 100 Hz. There is a notch filter at 50 Hz to suppress industrial interference in the electronics part of [
16]. Details and a block diagram, concerning associated electronics, of the TNB Antarctica Schumann measurement platform are presented by a research team from Italy [
17]. In the Schumann station located at Calar Alto (Spain), modes are captured through the 2-m magnetic antenna with an acquisition time of 30 min. Characterization of the sensor and detailed description of the amplification system are also presented [
13]. The magnetometers, noise of the system, and the ELF measurement station that has been deployed in Sierra Nevada (Spain) are described and discussed by five research teams from Spain and Sweden [
18]. The technical setup of the Hylaty geophysical station with a frequency range up to 300 Hz, as well as the design of ELF equipment, including antennas and receivers, is discussed by three research teams from Poland [
19]. In this paper, a versatile receiver for SR detection and monitoring is presented. The SR detection and monitoring system is portable, low-cost, battery-powered, autonomous for nearly 45 days’ time, and able to measure up to six SR harmonics. The system, which consists of the induction coil antenna and the amplifying and filtering chain as well as the data acquisition and processing system, was designed and implemented entirely in the Electronics-Telecommunications and Applications Lab (ETA Lab) of the Physics Department of the University of Ioannina. The constructed magnetic field antenna is much smaller than the antennas described in the literature with cores 0.8–2 m long and a diameter of a few centimeters. The magnetic field antenna is implemented by two back-to-back identical induction coils [
20] which are presented in detail and discussed in the following section. Moreover, the filtering and amplification chain exhibits an experimentally measured total passband gain equal to 410,000 or 112 dB (at 10 Hz). The preliminary induction coil sensor antenna design has already been presented and described [
21]. The design and implementation stages of the induction coil sensor were based on the fact that the induction core should avoid saturation due to external electromagnetic fields which were mostly originated from 50-Hz power lines. Therefore, the SR measuring equipment was installed in relatively low “EM pollution” areas. In order to evaluate the portable SR system, measurements were acquired at various spots which were located at 1-km far distances from man-made electromagnetic pollution in the area of Northwest Greece. From these measurements, it is obvious that up to six harmonics can be detected within 10-min acquisition time. Schumann resonance is a global phenomenon with numerous applications and many open questions [
22]. As already mentioned, there is a very limited number of ELF measurement stations around the globe, based on synchronous electronic methodologies and techniques of signal reception, conditioning, and processing. The contribution of this new ELF Schumann resonance receiver includes (a) signal conditioning stages with an equivalent input noise as low as 2.88 nV/√Hz and a total passband gain from 86 to 112 dB at 10 Hz, (b) monitoring and recording of six SR harmonics through a two back-to-back magnetic field antenna with total weight of 2.2 kg and 60 cm length, and (c) portability and over one and half month autonomy. Furthermore, discussion and detailed analysis of the efficient induction coil magnetic antenna and the low-noise amplifying-filtering chain through this work could motivate other researchers to create new and improved ELF measurement stations. The implemented induction coil antenna is presented and discussed in Section
2. The filtering and amplification chain we developed is extensively described in Section
3. Experimental results are present in Section
4, and finally, the article concludes with Section
5.