Studies on Endogenous Hormones and Nutritional Physiology Related to the Premature Senescence of Super-hybrid Rice Liangyoupeijiu and Its Parents at Late Growth Stage

The amount of root bleeding sap, contents of chlorophyl , nutrients and hormones in flag leaves of a super-hybrid rice cultivar Liangyoupeijiu （LYPJ） and its parents 9311 and Pei’ai 64S after heading were measured in this study. The re-sults revealed that compared with 9311, the chlorophyl content of LYPJ reduced more quickly after heading, and then kept at a lower level, which was an obvious characteristic of premature senescence. The other physiological indices of LYPJ af-ter heading except abscisic acid （ABA） content in leaf and root also maintained at a lower level than 9311, while al the physiological indices of the sterile line Pei＇ai 64S were lower than LYPJ. So it was speculated that the early-aging characteristic of LYPJ may be inherited from Pei’ai 64S. Al the leaf and root early-aging traits reduced for LYPJ and its parent lines after heading, their leaf and root aged grad-ual y, which indicated that the above-ground （leaf） and under-ground （root） parts cor-related to each other closely, but there was not absolute correlations between them judged from the data.

Characterization and evaluation of rice blast resistance of Chinese indica hybrid rice parental lines

The development of resistant varieties and hybrid combinations has been the most effective and economical strategy to control blast disease caused by Magnaporthe oryzae.However, the distribution of major R genes and blast resistance characterization in hybrid rice parents has not been well investigated, resulting in their limited use in hybrid rice blast-resistance breeding. In the present study, 88 elite indica hybrid rice parental lines were evaluated with 30 isolates of M. oryzae collected from the main planting area of indica hybrid rice in China and were characterized for the presence of 11 major resistance genes using molecular markers. The pathogenicity assays showed that four types of hybrid rice parent line showed some resistance to M. oryzae. However, the proportions of highly resistant lines and the mean resistance frequency(RF) varied among the four types, with resistance in decreasing order shown by three-line restorer lines, three-line maintainer lines, two-line sterile lines, and two-line restorer lines. All 88 hybrid rice parental lines carried more than one R gene, but none carried the R genes Pi1 and Pi2. Although Pid3 and Pi9 were present only in three-line restorer lines and Pigm only in three-line maintainer lines, the remaining six R genes(Pib, Pid2, Pi5, Pia, Pi54, and Pita) were present in the four types of hybrid rice parent with significantly different distribution frequencies. The correlation between R genes and resistance reactions was investigated. The results are expected to provide useful information for rational utilization of major R genes in hybrid rice breeding programs.

Increased grain yield with improved photosynthetic characters in modern maize parental lines

The grain yield of maize has increased continuously in past decades, largely through hybrid innovation, cultivation tech-nology, and in particular, recent genetic improvements in photosynthesis. Elite inbred lines are crucial for innovating new germplasm. Here, we analyzed variations in grain yield and a series of eco-physiological photosynthetic traits after anthesis in sixteen parental lines of maize (Zea mays L.) released during three different eras (1960s, 1980s, 2000s). We found that grain yield and biomass signiifcantly increased in the 2000s than those in the 1980s and 1960s. Leaf area, chlorophyl , and soluble protein content slowly decreased, and maintained a higher net photosynthesis rate (Pn) and improved stomatal conductance (Gs) after anthesis in the 2000s. In addition, the parental lines in the 2000s obtained higher actual photo-chemistry efifciency (ФPSI ) and the maximum PSII photochemistry efifciency (Fv/Fm), which largely improved light partition-ing and chlorophyl lfuorescence characteristic, including higher photochemical and photosystem II (PSII) reaction center activity, lower thermal energy dissipation in antenna proteins. Meanwhile, more lamel ae per granum within chloroplasts were observed in the parental lines of the 2000s, with a clear and complete chloroplast membrane, which wil greatly help to improve photosynthetic capacity and energy efifciency of ear leaf in maize parental lines. It is concluded that grain yield increase in modern maize parental lines is mainly attributed to the improved chloroplast structure and more light energy catched for the photochemical reaction, thus having a better stay-green characteristic and stronger photosynthetic capac-ity after anthesis. Our direct physiological evaluation of these inbred lines provides important information for the further development of promising maize cultivars.

Genetic Diversity among Parents of Hybrid Rice Based on Cluster Analysis of Morphological Traits and Simple Sequence Repeat Markers

The genetic diversity of 41 parental lines popularized in commercial hybrid rice production in China was studied by using cluster analysis of morphological traits and simple sequence repeat （SSR） markers. Forty-one entries were assigned into two clusters （i.e. early or medium-maturing cluster; medium or late-maturing cluster） and further assigned into six sub-clusters based on morphological trait cluster analysis, The early or medium-maturing cluster was composed of 15 maintainer lines, four early-maturing restorer lines and two thermo-sensitive genic male sterile lines, and the medium or late-maturing cluster included 16 restorer lines and 4 medium or late-maturing maintainer lines. Moreover, the SSR cluster analysis classified 41 entries into two groups （i.e, maintainer line group and restorer line group） and seven sub-groups. The maintainer line group consisted of all 19 maintainer lines, two thermo-sensitive genic male sterile lines, while the restorer line group was composed of all 20 restorer lines. The SSR analysis fitted better with the pedigree information. From the views on hybrid rice breeding, the results suggested that SSR analysis might be a better method to study the diversity of parental lines in indica hybrid rice.

Diurnal variation of gas exchange, chlorophyll fluorescence, and photosynthetic response of six parental lines of maize released in three eras

Over the past seven decades, the grain yield of maize(Zea mays L.) has increased continuously in China, mostly due to hybridization innovations, particularly recent genetic improvements in photosynthesis. In order to reveal photosynthetic characters of elite inbred lines in different ears, a field experiment was conducted at the North China Plain of Shandong Province in China. Six parental lines of maize introduced in three eras(the 1960 s, 1980 s, and 2000 s) were investigated diurnal variation of gas exchange, chlorophyll fluorescence, and photosynthetic response characteristic at the grain filling stage. Compared to earlier parental lines, the 2000 s parental lines always had higher net photosynthetic rate(Pn) throughout the day, especially at noon, and a mid-day depression in Pn did not occur in all hybrids parental lines. Moreover, the stomatal conductance(Gs) and water use efficiency(WUE) of the 2000 s’ lines showed higher value than those of the 1960 s’ and 1980 s’ lines. The inbred lines differences in photosynthetic parameters were partly owing to their different quantum carboxylation efficiencies and light synthase activities. Simultaneously, the 2000 s parental lines exhibited lower light and CO2 compensation points, and their higher apparent quantum yield, and carboxylation efficiency. These suggested that the modern parental lines required lower light intensity and less CO2 to maintain a relatively high photosynthetic capacity, substantially increasing leaf physical quality and stress resistance. It provided crucial information of high photo-efficiency and stress-resistance breeding in maize.

父母受教育程度对青年生育意愿的影响——基于中国家庭追踪调查(CFPS)数据的分析

青年生育意愿减弱是造成当前“超低生育率”问题的重要原因,而青年生育意愿的形成深受父母个人特征的影响。基于此,运用2018年中国家庭追踪调查(CFPS)数据,考察了父母受教育程度对青年生育意愿的影响机制。研究发现,父母受教育程度越高,青年的生育意愿越低;照料支持和“传宗接代”观念在父母受教育程度对青年生育意愿的影响过程中发挥了中介作用;经济帮助并非父母受教育程度对青年生育意愿产生代际影响的有效方式;相比于男性,女性的生育意愿更容易受到父母受教育程度的影响。在当前父母受教育程度不断提升的背景下,加强公共托幼服务,提供隔代照料津贴,培育积极生育观念和完善女性生育保障是提升青年生育意愿的有效政策措施。

一种监测母线槽的无线传感器信号采样策略

母线槽信号包含大量平稳信号和部分突发情况信号,完整准确地采集其信号能够保证母线槽的稳定运行。保持高上传率可准确地采集到信号,但功耗过大,降低设备使用寿命。文章提出一种适用母线槽信号的无线传感器节点近似采样策略(approximate sampling method,ASM),通过分析所采数据的相对变化程度及变化趋势捕捉完整突发情况信号,水塘抽样算法剔除部分无效平稳数据,完整准确地上传母线槽状态趋势信号。通过Matlab仿真表明ASM采样策略相比于SOD(send-on-delta)、无线传感器节点动态采样策略(dynamic sampling internal,DSI),无效采样率、变化偏移量更小,降低了能耗且保证了采样信号完整。

不同玉米杂交种及其亲本自交系耐热性的差异比较

【目的】近年来,我国黄淮海夏玉米区高温热害不利天气频发重发,已成为威胁玉米生产的重要不利因素。研究并明确高温胁迫对不同基因型玉米品种雌雄穗及产量的影响,为耐高温玉米品种培育和选择提供参考。【方法】以郑单958(郑58×昌7-2)、先玉335(PH6WC×PH4CV)、京农科728(京MC01×京2416)和MC812(京B547×京2416)及其亲本自交系为供试材料,花期前后(大喇叭口期-吐丝后7 d)进行高温胁迫处理,研究高温胁迫对不同基因型玉米杂交种及其亲本自交系雌雄穗生长发育、散粉吐丝间隔(ASI)、花粉活性、产量及其构成要素的影响。【结果】(1)花期前后高温胁迫导致参试玉米品种及其亲本自交系的穗粒数减少,进而产量降低,且不同品种和自交系对高温胁迫的响应存在显著差异。与对照相比,高温胁迫下,郑单958、先玉335、京农科728和MC812的穗粒数降幅分别为22.28%、46.79%、6.13%和8.11%,产量降幅分别为9.50%、50.61%、3.18%和5.00%,其中,京农科728和MC812减产不显著,而郑单958和先玉335显著减产;亲本自交系中,京2416的穗行数、行粒数和产量降幅最小且不显著,而PH6WC均显著降低且降幅最大。(2)高温胁迫下,参试品种及其亲本自交系的雄穗分支总数、雄穗长度、总散粉量和花粉活性降低,散粉持续期缩短,ASI延长。与对照相比,高温胁迫下,ASI延长1.6 d。雄穗长度降幅表现为郑单958>先玉335>MC812>京农科728。郑单958雄穗长度降幅最大,但雄穗分支数多,花粉量最大;先玉335雄穗分支少,雄穗长度降幅大,花粉量最少且活性最低;京2416总散粉量大且花粉活力强,降幅最小(仅为4.50%和3.98%)。【结论】花期前后高温胁迫对参试玉米品种的籽粒产量和花粉活性等影响较大,京农科728和MC812的产量和花粉活性降幅显著低于先玉335和郑单958,耐热性较好。通过比较参试玉米杂交种亲本自交系的耐热性,父本自交系的耐热性要好于母本自交系。其中,京2416的雄穗分支和长度降幅小,花粉量大,花粉活性高,且花丝茸毛多,捕获花粉能力强,单穗产量高,ASI小,耐热性最好。因此,在耐高温玉米品种选育过程中,要重视和加大对耐热种质(如京2416等)的利用与改良创新,组配选育耐高温玉米新品种。

高温胁迫对玉米杂交种及其亲本自交系光合特性、保护酶活性和产量的影响

研究并明确高温胁迫对玉米杂交种及其亲本自交系叶片光合性能、产量性状等的影响,以期为耐高温玉米品种选育和推广提供理论依据。以‘京农科728’‘MC812’‘先玉335’和‘郑单958’及其亲本自交系为试验材料,于花期前后(大喇叭口期—吐丝后7 d)对其进行高温胁迫(高温胁迫15 d)处理,研究高温胁迫对不同基因型玉米杂交种及其亲本自交系叶绿素相对含量、光合特性、最大光化学效率(F_(v)/F_(m))、保护酶活性、产量及其产量构成要素的影响。结果表明:1)与大田对照相比,花期前后高温胁迫下不同杂交种及其亲本自交系的叶绿素相对含量、净光合速率、气孔导度和F_(v)/F_(m)均呈降低趋势,杂交种以‘京农科728’降幅最小,亲本自交系以‘京2416’降幅最小。胞间CO_(2)浓度和蒸腾速率则均呈升高趋势,杂交种以‘京农科728’增幅最小,亲本自交系以‘京2416’增幅最小。2)花期前后高温胁迫导致玉米杂交种及其亲本自交系的穗位叶磷酸烯醇式丙酮酸羧化酶(PEPCase)、核酮糖-1,5-二磷酸羧化酶(RuBPCase)、过氧化氢酶(CAT)和超氧化物歧化酶(SOD)活性呈降低趋势。3)花期前后高温胁迫降低了玉米杂交种及其亲本自交系的穗行数和行粒数,进而导致产量下降,杂交种‘京农科728’‘MC812’‘先玉335’和‘郑单958’产量分别降低3.18%、5.00%、50.61%和9.50%;亲本自交系中,‘京2416’的穗行数、行粒数和产量降幅最小,而‘PH6WC’产量降幅最大。由此可见,花期前后高温胁迫下‘京农科728’‘MC812’及其父本自交‘京2416’具有较高的叶绿素相对含量、光合能力和保护酶活性,产量受高温影响较小,具有较好的耐热性。

Discovery of a variable broad absorption line in the BL Lac object PKS B0138-097

We report the discovery of a broad absorption line （BAL） of - 10^4 km s^-1 in width in the previously known BL Lac object PKS 0138-097, which we tentatively identified as an Mg II BAL. This is the first detection of a BAL, which is sometimes seen in powerful quasars with high accretion rates, in a BL Lac object. The BAL was clearly detected in its spectra spanning two epochs at a high luminosity state taken in the Sloan Digital Sky Survey （SDSS）, while it disappeared in three SDSS spectra taken at a low luminosity state. The BAL and its variability pattern were also found in its historical multi-epoch spectra in the literature, but have been overlooked previously. In its high resolution radio maps, PKS 0138-097 shows a core plus a one- sided parsec-scale jet. The BAL variability can be interpreted as follows： The optical emission is dominated by the core in a high state and by the jet in a low state and the BAL material is located between the core and jet so that the BAL appears only when the core is shining. Our discovery suggests that outflows may also be produced in active galactic nuclei at a low accreting state.

Estimating Black Hole Masses of AGNs using Ultraviolet Emission Line Properties

Based on measured broad line region sizes in the reverberation-mapping AGN sample, two new empirical relations are introduced to estimate the central black hole masses of radio-loud high-redshift （z 〉 0.5） AGNs. First, using the archival IUE/HST spectroscopy data at UV band for the reverberation-mapping objects, we obtained two new empirical relations between the BLR size and Mg Ⅱ/C Ⅳ emission line luminosity. Secondly, using the newly determined black hole masses of the reverberation-mapping sample as calibration, we found two new relationships for determining the black hole mass with the full width at half maximum and the luminosity of Mg Ⅱ/C Ⅳ line. We then apply the relations to estimate the black hole masses of the AGNs in the Large Bright Quasar Survey and a sample of radio-loud quasars. For the objects with small radio-loudness, the black hole mass estimated using the RBLR-LMg Ⅱ/C Ⅳ relation is consistent with that from the RBLR-L3000 A/1350 A relation. For radio-loud AGNs, however, the mass estimated from the RBLR-LMg Ⅱ/C Ⅳ relation is systematically lower than that from the continuum luminosity L3000 A/13S0 A Because jets could have significant contributions to the UV/optical continuum luminosity of radio-loud AGNs, we emphasize once again that for radio-loud AGNs, the emission line luminosity may be a better tracer of the ionizing luminosity than the continuum luminosity, so that the relations between the BLR size and UV emission line luminosities should be used to estimate the black hole masses of high redshift radio-loud AGNs.

A search for double-peaked narrow emission line galaxies and AGNs in the LAMOST DR1

The Large Sky Area Multi-Object Fiber Spectroscopic Telescope （LAMOST） has released more than two million spectra, which provide the opportunity to search for double-peaked narrow emission line （NEL） galaxies and active galactic nuclei （AGNs）. The double-peaked narrow-line profiles can be well modeled by two velocity components, respectively blueshifted and redshifted with respect to the sys- temic recession velocity. This paper presents 20 double-peaked NEL galaxies and AGNs found from LAMOST DR1 using a search method based on a multi-Gaussian fit of the narrow emission lines. Among them, ten have already been published by other authors, either listed as genuine double-peaked NEL objects or as asymmetric NEL objects, and the remaining ten are original discoveries. We discuss some pos- sible origins for the double-peaked narrow-line features, such as interaction between jet and narrow line regions, interaction with companion galaxies, and black hole bina- ries. Spatially resolved optical imaging and/or follow-up observations in other spectral bands are needed to further discuss the physical mechanisms at work.

Strong optical and UV intermediate-width emission lines in the quasar SDSS J232444.80–094600.3:dust-free and intermediate-density gas at the skin of dusty torus?

Emission lines from the broad emission line region （BELR） and the narrow emission line region （NELR） of active galactic nuclei （AGNs） have been extensively studied. However, emission lines are rarely detected between these two regions. We present a detailed analysis of quasar SDSS J232444.80-094600.3 （SDSS J2324-0946）, which is remarkable for its strong intermediate-width emission lines （IELs） with FWHM ≈ 1800 km s^-1. The IEL component is present in different emission lines, including the permitted lines Lyαλ1216, CⅣ λ1549, semiforbidden line C Ⅲ] λ1909, and forbidden lines [OⅢ] ss4959, 5007. With the aid of photo-ionization models, we found that the IELs are produced by gas with a hydrogen density of nH - 10^6.2 -- 10^6.3 cm^-3, a distance from the central ionizing source of R - 35 - 50 pc, a covering factor of - 6%, and a dust-to-gas ratio of ≤ 4% that of the SMC. We suggest that the strong IELs of this quasar are produced by nearly dust-free and intermediate-density gas located at the skin of the dusty torus. Such strong IELs, which serve as a useful diagnostic, can provide an avenue to study the properties of gas between the BELR and the NELR.

Discovery of Balmer broad absorption lines in the quasar LBQS 1206+1052

We report the discovery of Balmer broad absorption lines （BALs） in the quasar LBQS 1206＋1052 and present a detailed analysis of the peculiar absorption line spectrum. Besides the Mg II λλ2796, 2803 doublet, BALs are also detected in the He I＊ multiplet at λλ2946, 3189, 3889 A arising from the metastable helium 2 3 S level, and in Hα and Hβ from the excited hydrogen H I＊ n = 2 level, which are rarely seen in quasar spectra. We identify two components in the BAL troughs of v ～ 2000 km s 1 width： One component shows an identical profile in H I＊, He I＊ and Mg II with its centroid blueshifted by v c ≈ 726 km s-1 . The other component is detected in He I＊ and Mg II with v c ≈ 1412 km s-1 . We estimate the column densities of H I＊, He I＊, and Mg II, and compare them with possible level population mechanisms. Our results favor the scenario that the Balmer BALs originate in a partially ionized region with a column density of N H ～ 10 21 10 22 cm-2 for an electron density of n e ～ 10 6 10 8 cm-3 via Lyα resonant scattering pumping. The harsh conditions needed may help to explain the rarity of Balmer absorption line systems in quasar spectra. With an i-band PSF magnitude of 16.50, LBQS 1206＋1052 is the brightest Balmer-BAL quasar ever reported. Its high brightness and unique spectral properties make LBQS 1206＋1052 a promising candidate for followup high-resolution spectroscopy, multi-band observations, and long-term monitoring.

Line profile studies of hydrodynamical models of cometary compact H II regions

We simulate the evolution of cometary H II regions based on several champagne flow models and bow shock models, and calculate the profiles of the [Ne II] fine-structure line at 12.81 μm, the H30α recombination line and the [Ne III] finestructure line at 15.55 μm for these models at different inclinations of 0°, 30° and 60°. We find that the profiles in the bow shock models are generally different from those in the champagne flow models, but the profiles in the bow shock models with lower stellar velocity （≤ 5 km s^-1） are similar to those in the champagne flow models. In champagne flow models, both the velocity of peak flux and the flux weighted central velocities of all three lines point outward from molecular clouds. In bow shock models, the directions of these velocities depend on the speed of stars. The central velocities of these lines are consistent with the stellar motion in the high stellar speed cases, but they are opposite directions from the stellar motion in the low speed cases. We notice that the line profiles from the slit along the symmetrical axis of the projected 2D image of these models are useful for distinguishing bow shock models from champagne flow models. It is also confirmed by the calculation that the flux weighted central velocity and the line luminosity of the [Ne III] line can be estimated from the [Ne II] line and the H30α line.

春播早熟区高粱杂种优势群及杂种优势模式分析

杂种优势群的划分对于拓宽亲本间遗传基础、提高育种效率,培育突破性新品种具有重要的指导作用。本研究利用全基因组重测序技术对55份春播早熟区40余年生产中主推杂交种亲本系进行全基因组扫描,分析其群体结构,估算遗传距离,划分杂种优势群,分析主推杂交种的杂种优势模式。结果表明,利用全基因组5×测序,过滤到1,304,623个高质量SNP标记用于群体结构分析和杂种优势类群划分。55份高粱亲本系平均遗传距离为0.704,变幅0.627~0.927。多态信息含量(polymorphism information content,PIC)平均为0.2935,变幅为0.1~0.5。群体结构和主成分分析将55份亲本系划分为4个杂种优势群:都拉群(Durra,D群)、卡佛尔/都拉群(Kafir/Durra,KD群)、俄罗斯/卡佛尔群(Russia/Kafir,RK群)、中国高粱群(Kaoliang,K群)。25个主推杂交种中76%的杂交种杂种优势模式为Kafir/Durra×Kaoliang模式,主推高粱杂交种的不育系主要来源于引自国外的Kafir和Durra群,恢复系多来源于我国自产的Kaoliang群。本研究的群体结构分析及其划分的杂种优势群阐明了春播早熟区高粱亲本系的遗传基础,为亲本系改良和杂种优势模式创新研究提供科学依据。

The broad wing of the [O Ⅲ] λ5007 emission line in active galactic nuclei

We use a sample of type 2 active galactic nuclei （AGNs） from SDSS DR7 in which the [O Ⅲ] ）λ5007 emission line can be modeled by two Gaussian components, a broad wing plus a narrow core, to investigate the origin of the broad wing and the connection between the velocity shift of the broad wing and the physical parameters of AGNs, as well as their host galaxies. We find that the flux of the wing components is statistically roughly equal to that of the core components. However, the velocity shift of the wing component has only weak, if any, correlations with the physical properties of AGNs and the host galaxies, such as bolometric luminosity, the Eddington ratio, the mass of supermassive black holes, D4000, H3A or stellar mass. Comparing the velocity shift from our type 2 AGN sample to that from the type 1 sample in Zhang et al., we suggest that the [O Ⅲ]] broad wing originates from outflow.

Near-infrared studies of nova V5584 Sgr in the pre-maximum and early decline phase

We present near-infrared spectroscopic and photometric observations of nova V5584 Sgr taken during the first 12 d following its discovery on Oct. 26.439 UT2009. The evolution of the spectra is shown from the initial P Cygni phase to an emission line phase. The prominent carbon lines seen in the JHK spectra closely match those observed in an Fe II class nova outburst. The spectra show first-overtone CO bands in emission between 2.29-2.40 μm. By examining WISE and other publicly available data, we show that the nova underwent a pronounced dust formation phase between February- April 2010.

X-ray Emission Lines in GRB Afterglows: Evidence for a Two-component Jet Model

X-ray emission lines have been observed in X-ray afterglows of several T-ray bursts （GRBs）. It is a major breakthrough for understanding the nature of the progenitors. It has been proposed that the X-ray emission lines can be well explained by the Geometry-Dominated models, but in these models the illuminat- ing angle is much larger than that of the collimated jet of the GRB. For GRB 011211, we have obtained an illuminating angle of about 0 - 45°, while the angle of the GRB jet is only 3.6°. So we propose that the outflow of GRBs with emission lines should have two distinct components： a wide component that illuminates the reprocessing material and produces the emission lines and a narrow one that produces the GRB. Observations show the energy for producing the emission lines is higher than that of the GRB. In this case, when the wide component dominates the afterglows, a bump should appear in the GRB afterglow. For GRB 011211, the bump should occur within 0.05 days of the GRB, which is obviously too early for the observation to catch it. Alongside the X-ray emission lines there should also be a bright emission component between the UV and the soft X-rays. These features can be tested by the Swift satellite in the near future.

父母本行比和播期对青花菜“台绿5号”制种产量的影响

为了增加青花菜台绿5号的制种产量,研究了不同父母本行比(父本:母本=1:1、父本:母本=2:1)和母本播期(8月10日、8月20日)对制种产量及相关性状的影响。结果表明:制种时父母本2:1处理的单株有效荚数为735.13荚、每荚粒数为2.04粒、折合667 m2产量为6.42 kg,分别极显著高于父母本1:1处理的362.42荚、1.31粒、2.35 kg;2个母本播期处理对制种产量及相关性状的影响不显著,但从父母本花期的相遇时间来看,母本播期选择8月10日更合适。因此,建议在台绿5号制种时选择父母本行比为2:1,母本播期以8月10日为宜。