ALBERT

All Library Books, journals and Electronic Records Telegrafenberg

feed icon rss

Your email was sent successfully. Check your inbox.

An error occurred while sending the email. Please try again.

Proceed reservation?

Export
  • 1
    ISSN: 1573-5036
    Keywords: Brassica napus ; H ion efflux ; nitrate accumulation ; nitrate reductase ; phosphate nutrition ; xylem exudation
    Source: Springer Online Journal Archives 1860-2000
    Topics: Agriculture, Forestry, Horticulture, Fishery, Domestic Science, Nutrition
    Notes: Abstract Levels of nitrate reductase activity (N.R.A.) were measured in shoots and roots of P sufficient and P deficient rape plants and changes in N.R.A. examined in relation to the onset of H ion efflux from the roots. Rates of xylem exudation were measured and the sap analysed for nitrate, amino-N and phosphate content. The optimum concentration of phosphate in the leaves for N.R.A. was about 0.7%. Both high and low concentrations of phosphate within the leaves inhibited N.R.A in those leaves. This inhibition of N.R.A led to the accumulation of nitrate in the older parts of the shoots of P sufficient plants. Less accumulation of nitrate occurred in the P deficient plants since nitrate uptake by the plants decreased before any fall in N.R.A. Xylem exudation rates halved within 18 hours of depriving the plants of phosphate, and, since the composition of the sap remained constant, this indicated a reduced flux of nitrate into the xylem. The rate of xylem exudation continued to fall and by the end of the experiment was approximately one tenth of the rate in the P sufficient plants. The onset of H ion efflux from the terminal portions of the root preceded any effect on N.R.A by 2 days.
    Type of Medium: Electronic Resource
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 2
    Electronic Resource
    Electronic Resource
    Springer
    Plant and soil 105 (1988), S. 247-256 
    ISSN: 1573-5036
    Keywords: Brassica napus ; cation-anion balance ; H ion efflux ; phosphate nutrition ; root growth
    Source: Springer Online Journal Archives 1860-2000
    Topics: Agriculture, Forestry, Horticulture, Fishery, Domestic Science, Nutrition
    Notes: Abstract Changes in pH around the roots of young rape plants were studied using a nutrient film technique which allowed either part or all of the root system to be subjected to specific nutrient treatments. The rapidity and direction of change of pH was assessed by embedding absorbing roots in a thin layer of agar containing bromocresol purple. Measurements were also made with a pH microelectrode placed next to the roots. Phosphate-fed plants were deprived of phosphate when 14 days old. Patterns of pH changes round the deprived roots were the same as with phosphate-fed plants until the plants had been deprived of P for three days, when H ion efflux started in the terminal portions of the roots. The lengths of root producing acid and amounts of H ion both increased as the plants became more P deficient. Both P fed and P deprived roots produced HCO3 ions but the net amount of HCO3 ion produced by the P deficient roots fell as did nitrate uptake rates. Cation-anion balances measured at the end of the experiment showed that uptake of all anions and K decreased in the P deprived plants but uptake of Ca and Mg were little altered. This resulted in a smaller ratio of anions to cations absorbed which was reflected in the reduced HCO3 ion efflux.
    Type of Medium: Electronic Resource
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 3
    Electronic Resource
    Electronic Resource
    Springer
    Plant and soil 84 (1985), S. 403-415 
    ISSN: 1573-5036
    Keywords: Agar-pH indicator technique ; Cation-anion balance ; H ion efflux ; HCO3 ; ion efflux ; Nitrate nutrition ; Nitrate reductase ; Root growth ; Split root system
    Source: Springer Online Journal Archives 1860-2000
    Topics: Agriculture, Forestry, Horticulture, Fishery, Domestic Science, Nutrition
    Notes: Summary Changes in pH around the roots of young rape plants (Brassica napus cv. emerald) were studied using a nutrient film technique that allowed part or whole of the root system to be subjected to specific nutrient treatments. The rapidity and direction of pH change was assessed by imbedding absorbing roots in a thin film of agar containing bromocresol purple. When nitrate-fed plants were deprived of all sources of nitrogen at 15 or 17 days old, the release of H ions from the roots was immediate and uniformly distributed over the root length. When nitrate was witheld from half of the root system of nitrate-fed plants, the roots deprived of nitrate immediately started to produce H ions even though the nitrate-fed half of the root system continued to supply the whole of the plant with nitrate. However, the rate of H ion production in plants partly supplied with NO3 was less than in plants completely deprived of NO3. It is suggested that malate produced in the shoots, following nitrate reduction, may be redistributed to the roots deprived of nitrate. There, HCO3 produced by the decarboxylation of the malate masks some of the expected H ion efflux.
    Type of Medium: Electronic Resource
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 4
    Publication Date: 2011-08-16
    Description: Wavelengths of the Hg II absorption feature at 3984 A in 30 Hg stars are distributed uniformly from the value for the terrestrial mix to a value that corresponds to nearly pure Hg-204. The wavelengths are correlated loosely with effective temperatures inferred from Q(UBV). Relative isotopic abundances derived from partially resolved profiles of the 3984-A line in iota CrB, chi Lup, and HR 4072 suggest that mass-dependent fractionation has occurred in all three stars. It is supposed that such fractionation occurs in all Hg stars, and a scheme whereby isotopic compositions can be inferred from a comparison of stellar wavelengths and equivalent widths with those calculated for a family of fractionated isotopic mixes. Theoretical profiles calculated for the derived isotopic composition agree well with high-resolution interferometric profiles obtained for three of the stars.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal; 204; Feb. 15
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 5
    Publication Date: 2016-06-07
    Description: Although there is a large amount of interstellar matter near the Pleiades star cluster, the observed dust and gas is not a remnant of the placental molecular cloud from which the star cluster was formed. Carbon monoxide (CO) associated with the visible reflection nebulae was discovered by Cohen (1975). Its radial velocity differs from that of the cluster by many times the cluster escape velocity, which implies that the cloud-cluster association is the result of a chance encounter. This circumstance and the proximity of the Pleiades to the sun creates an unique opportunity for study of interstellar processes at high spatial resolution. To study the molecular component of the gas, a 1.7 square degree field was mapped with the AT&T Bell Laboratories 7-meter antenna (1.7' beam) on a 1' grid in the J=1.0 C(12)O line, obtaining over 6,000 spectra with 50 kHz resolution. The cloud core was mapped in the J=1-0 line of C(13)O. Further observations include an unsuccessful search for CS (J=2-1) at AT&T BL, and some C(12)O J=2-1 spectra obtained at the Millimeter Wave Observatory of the University of Texas.
    Keywords: ASTROPHYSICS
    Type: NASA. Ames Research Center Summer School on Interstellar Processes: Abstracts of Contributed Papers; p 51-52
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 6
    Publication Date: 2011-08-18
    Description: Observations of interstellar absorption in the resonance doublet 7664, 7698 A of neutral potassium toward 188 early-type stars at a spectral resolution of 8 km/s are reported. The 7664 A line is successfully separated from nearly coincident telluric O2 absorption for all but a few of the 165 stars for which K I absorption is detected, making possible an abundance analysis by the doublet ratio method. The relationships between the potassium abundances and other atomic abundances, the abundance of molecular hydrogen, and interstellar reddening are investigated.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal Supplement Series; 50; Oct. 198
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 7
    Publication Date: 2019-06-27
    Description: Microturbulence and systematic motions are viewed as simplifying assumptions made to facilitate treatment of line formation in molecular clouds, and line intensities calculated in the two approximations are compared to estimate how uncertainties about the actual line-broadening mechanism affect the interpretation of molecular emission lines. For lines formed by two-level molecules in an isothermal homogeneous cloud, the alternative assumptions lead to peak and integrated line intensities which agree within the differences (up to a factor of 3) associated with the ignorance of cloud geometry. New multilevel calculations for CO in the same cloud model bear out the generality of this result. It follows that, within the geometrical uncertainties, the Sobolev (1960) approximation may be used confidently in the numerous applications for which this simple cloud model suffices.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal; vol. 211
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
Close ⊗
This website uses cookies and the analysis tool Matomo. More information can be found here...