† Corresponding author. E-mail:
Project supported by the Strategic Pioneer Program on Space Science, Chinese Academy of Sciences (Grant Nos. XDA15010800 and XDA15320102) and the National Natural Science Foundation of China (Grant Nos. 11427901, 11773040, 11403047, and 11427803).
The Advanced Space-based Solar Observatory (ASO-S) is a mission proposed by the Chinese Solar Physics Community. As one of the three payloads of ASO-S, the Full-disc Magneto-Graph (FMG) will measure the photospheric magnetic fields of the entire solar disk with high spatial and temporal resolution, and high magnetic sensitivity, where liquid crystal variable retarder (LCVR) is the key to whether FMG can achieve its scientific goal. So far, there is no space flight experience for LCVR. Therefore, irradiation study for LCVRs becomes more important and urgent in order to make sure their safety and reliability in space application. In this paper, λ irradiation, proton irradiation, and ultra-violet (UV) irradiation are tested for LCVRs respectively. The optical and chemical properties during irradiation tests are measured and analyzed. For optical properties, there is no significant change in those parameters FMG payload concerned except the retardation. Although there is no drastic degradation in the retardation versus voltage during irradiations, the amount of retardation variation is much higher than the instrument requirements. Thus, an in-flight retardation versus voltage should be added in FMG payload, reducing or even avoiding the impact of retardation change. For chemical properties, the clearing point and birefringence of the LC materials almost have no change; the ion density dose not change below 60 krad[Si], but begin to increase dramatically above 60 krad[Si].
The Advanced Space-based Solar Observatory (ASO-S)[1] is a mission proposed for the 25th solar maximum by the Chinese Solar Physics Community. This mission is supported by the Chinese Academy of Sciences (CAS) Strategic Pioneer Program on Space Science and is scheduled to be launched at the end of 2021 or early 2022.
Being the first approved Chinese Solar Satellite, ASO-S will focus on observing solar magnetic fields, solar flares, and coronal mass ejections (CMEs) simultaneously, in order to study the relationships between the solar magnetic field, solar flares, and CMEs, which are the key scientific questions in modern solar physics.[2–5] Where the magnetic field is the preferred physical parameter measured by ASO-S. As one of three payloads, the Full-disc Magneto-Graph (FMG) will measure the photospheric magnetic fields of the entire solar disk with high spatial and temporal resolution, and high magnetic sensitivity.[2]
Solar magnetic field, especially in photosphere, is measured by polarimetry based on Zeeman effect and polarized radiation transfer theory of solar atmosphere.[6,7] Thus, solar magnetic field measurement is actually a polarization measurement for solar telescopes, and polarimetry is the key to magnetic field measurement by solar telescopes,[8–13] no exception for FMG.
FMG is a full-disk vector magnetic fields telescope with an aperture 140 mm and working spectra line Fe I 532.4 nm. Both liquid crystal variable retarders (LCVRs) are utilized in Stokes polarimeter of FMG to improve polarization sensitivity. LCVR is envisaged as a promising novel technique for polarization measurement in space applications due to the inherent advantage of eliminating the need for conventional rotating polarizing optics and increasing the measuring speed.[14,15] However, any onboard element used for aerospace applications must be space qualified; i.e., it must be able to survive the hazards of operation in space due to harsh space radiation environmental conditions, and it must be low risk. So far, there is no space flight experience for LCVRs, therefore irradiation tests for LCVRs become more important than traditional mechanic mode.
A few irradiation tests have been done in the past to verify the spatial adaptability of LCVRs.[16–23] Heredero, Patarroyo, Belenguer et al.[16] have done the λ and UV irradiations tests of LCVRs in 2007 for the Imaging Magnetograph eXperiment (IMaX), which is one of the three instruments of the payload of the SUNRISE balloon project within the NASA Long Duration Balloon program. Herrero, Patarroyo and Parejo et al. reported λ, proton, and UV irradiations tests of LCVRs in 2011 for Solar Orbiter space mission.[17] However, no driving voltage had been applied to LCVRs in these irradiation tests. But for an elctro-optic modulation device, the irradiation characteristic of LCVRs with and without derived voltages during irradiations is also a key point needed to research.
In this paper, the radiation effects of LCVRs used in FMG payload are systematically studied. The main purpose of this study is to test and analyze whether the performance changes of LCVRs under various irradiations can meet the scientific requirements of FMG, and to give the corresponding strategies. The results are also expected to be helpful to developing some other relevant LCVRs-based aerospace instruments.
An LCVR consists of a nematic liquid-crystal (LC) material layer sandwiched between two fused-silica substrates (illustrated in Fig.
Table
ASO-S will be launched to a Sun-synchronous orbit (SSO) at an attitude of 720 km. The harsh space environments on the orbit are the radiation belts protons, the radiation belts electrons, solar protons, UV radiation, atomic oxygen, and space debris. It is difficult for atomic oxygen and space debris to get inside of optic box of FMG, so what we need to consider is the influence of the radiation belts protons, the radiation belts electrons, solar protons and UV radiation on LCVRs. According to the structure characteristics and operating principle of LCVR and analysis of environmental effects of space radiation, the possible impacts and dose are as follows.
Energy will be deposited when high-energy protons and electrons pass through LCVR, which will lead to the ionization of nearby atoms and produce electrons and ions. The energy is total ionization dose. The poor conductivity of LCVR makes the electrons and ions difficult to rapidly compound, and then a new electric dipole moment is formed within LCVR. The new electric dipole moment may affect the effective voltage added to LCVR, thus changing the relations of phase retardation with derived voltages. The total ionization dose incidence in LCVR is about 9.6 krad[Si] and 20.7 krad[Si] at 5-year and 11-year respectively, where 5-year is the ASO-S design lifetime and 11-year is a solar cycle we hope ASO-S can work.
The collision between high-energy protons and molecules of liquid crystal materials may lead to the displacement of atoms, changing the properties of LCVR. The energy doposied by the collision is the displacement damage dose. The dose of displacement damage of LCVR is 2.4 × 108 MeV/g and 5.3 × 108 MeV/g at 5-year and 11-year, respectively.
High-energy electrons are deposited in the liquid crystal material or on the substrate of LCVR, which will lead to the continuous accumulation of electrons and form the charging effect. The charging will counteract or enhance the applied voltage when the LCVR works, hence changing the polarization characteristics of LCVR. The equilibrium potential of charging is about 1.8 × 10−6 V after calculation, which is far less than the required voltage accuracy 0.001 V of LCVR. The possible reason is that our satellite orbit is relatively low and the flux of high-energy electrons on the LCVR is so small that the charging effect is week. But the effect has to be focused on high orbit as geosynchronous orbit.
Because FMG is a solar telescope, UV radiation must be taken into account. Moreover, LC material is also sensitive to UV spectra. The ultraviolet irradiation may change the chemical properties of LCVR, leading to performance degradation. In order to reduce the influence of UV radiation and stray light on FMG, a front widow with a pass band 532.4 nm±5 nm is designed and used to prevent the light from other wavelengths entering the optical system. The transmittance of front window is given Fig.
Table
A total of twelve identical LCVRs were used for irradiation testing: four LCVRs for λ irradiation (LCVR#1–LCVR#4), three for proton irradiation (LCVR#5–LCVR#7), and four for UV irradiation (LCVR#8–LCVR#11). The remaining one sample (LCVR#12) was designated as controls and was not exposed to any irradiation but was shipped between locations together with the irradiation samples to make their history as similar as possible. Besides, seven identical liquid crystal (LC) materials were exposed to λ irradiation to test the material’s chemical properties.
To verify the fulfilment of LCVRs requirements for FMG the following seven key parameters were measured in irradiation experiments:
Retardation versus voltage; Response time; Transmission; Transmitted wavefront error; Clearing point; Birefringence; Ion concentration.
The first four parameters represent the optical properties of LCVRs and the last three represent the chemical properties of LC material we used.
All the parameters were not measured in situ. In each irradiation, parameters (i)–(iii) had to be measured during all the intermediate doses, the time-lapse from the start of the optical parameters measurements to the start of the next irradiation exposure (another intermediate doses) is limited to one hour. By contrast, parameter (iv) was measured only before and after each irradiation test and parameters (iv)–(vii) measured only after γ irradiation test.
The experimental setups employed to measure all the optical parameters included an automatic retardation-voltage measurement system that can measure retardation–voltage curves and response time, a transmission measuring system with fiber-spectrometer and a Zygo interferometer. Response time was required to measure at 35°C where LCVRs work in FMG. The other parameters were measured in room temperature.
The LCs samples after γ irradiation were measured by Xi’an Modern Chemistry Research Institute to test the chemical change of LCVRs, including clearing point and birefringence and ion concentration.
It is noted that, a simple, fast but robust method was applied to measure retardation–voltage curves in the automatic retardation–voltage measurement system as shown in Fig.
The γ irradiation was tested in Peking University (Fig.
The proton irradiation was tested at 100-MeV compact cyclotron (CYCIAE-100) in China Institute of Atomic Energy (Fig.
The UV irradiation was tested in Harbin Industrial University (as shown in Fig.
Tables
Figure
In order to analyze these changes in detail we got the retardation variation curves with irradiation dose for every sample by only extracting one voltage point from each sample. The voltage value chosen corresponds to the retardation about 360°, which is the most sensitive position to irradiation over the retardation range of 90°–360° and can completely represent the trend of the whole retardation–voltage curve we need. The results are shown in Fig.
The first row in Fig.
The second row shows the retardation and variation rates measured after the LCVRs have been irradiated by proton with 5 × 1010, 10 × 1010, 20 × 1010, 50 × 1010, and 100 × 1010 p/cm2. It can be found that: i) All the samples have the same trend with proton dose no mater with voltage or not during irradiation; ii) The larger the dose, the slower the rate of change; iii) The retardation of the sample with voltage during irradiation changes about 11.1%, almost twice as large as those of samples without voltage; iv) The retardation changes rapidly before 10 × 1010 p/cm2, then it reaches saturation but can return to original value after completing proton irradiation (measured again three days after the end of the irradiation).
The last two rows show the retardation and variation rates measured after the LCVRs have been irradiated by UV light in the spectra ranges of [200 400] nm and [360 400] nm respectively. The main results are the following ones: A strange phenomenon is found that the retardation goes through two cycles of increase and decrease. The largest change is about 4.2%. The retardation measured 12 hours after the end of the UV irradiation has a tendency trying to return to its original state.
The response time is defined as the time needed for the LCVR to reach a second polarization state defined by voltage applied to the LCVR V1 from the first polarization state defined by voltage V2.
In irradiation testing, the exposure time is 1 ms; V1 and V2 are set in 2 V and 5 V respectively, which corresponds to the retardation about 360° and 90°. The measured results are shown in Fig.
It is observed that: the rising time from V1 to V2 (< 32 ms) is significantly less than the falling time from V2 to V1 (< 50 ms). There are three typical response times found in the measurements, 16 ms, 32 ms, and 47 ms. They are almost multiple relationships, which are very interesting phenomena that deserve further study. However, there was no obvious change in response time before and after the irradiation test. The response time is less than 50 ms, meeting the scientific requirements of FMG payload.
Figure
The main results for wavefront error of all the samples can be seen in Table
Tables
For optical properties of LCVR, error requirements for LCVR are listed in Table
For chemical properties of LCVR, the measured results in Tables
In this paper, space radiation effects and the equivalent dose of LCVR in FMG were analyzed and calculated firstly; based on that, λ irradiation, proton irradiation, and UV irradiation were tested for LCVRs respectively. The optical and chemical properties during irradiation tests were measured and analyzed. Some results are given below.
(I) For optical properties, there is no significant change in those parameters for FMG payload concerned except the retardation.
(II) For retardation, the amount of retardation change is still much higher than the instrument requirements though there is no drastic change in the retardation versus voltage during three irradiation processes.
(III) For chemical properties, the clearing point and birefringence of the LC materials almost have no change; the ion density does not change below 60 krad[Si], but begins to increase dramatically above 60 krad[Si].
Besides, some more interesting phenomena are also found:
The retardation changes in proton irradiation are obviously larger than those in λ and UV irradiations; the retardation of the samples with voltage during proton irradiation changes about 11.1%, almost twice as large as those of samples without voltage. The retardation measured after the end of the proton and UV irradiations has a tendency trying to return to its original state. The most possible reason is that the irradiations mainly alter the effective electric field inside LCVR. After the irradiation is finished, the retardation gradually reverts to the initial value with the attenuation of the additional electric field. There are three typical response times found in the measurements, 16 ms, 32 ms, and 47 ms. They are almost multiple relationships, which are very interesting phenomena that deserve further study.
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[5] | |
[6] | |
[7] | |
[8] | |
[9] | |
[10] | |
[11] | |
[12] | |
[13] | |
[14] | |
[15] | |
[16] | |
[17] | |
[18] | |
[19] | |
[20] | |
[21] | |
[22] | |
[23] |